The linear algebra a beginning graduate student ought to know

THE LINEAR ALGEBRA A BEGINNING GRADUATE STUDENT OUGHT TO KNOW The Linear Algebra a Beginning Graduate Student Ought t...

Author: Golan J.S.

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THE LINEAR ALGEBRA A BEGINNING GRADUATE STUDENT OUGHT TO KNOW

The Linear Algebra a Beginning Graduate Student Ought to Know Second Edition

by

JONATHAN S. GOLAN University of Haifa, Israel

A C.I.P. Catalogue record for this book is available from the Library of Congress.

ISBN-10 ISBN-13 ISBN-10 ISBN-13

1-4020-5494-7 (PB) 978-1-4020-5494-5 (PB) 1-4020-5495-5 (e-book) 978-1-4020-5495-2 (e-book)

Published by Springer, P.O. Box 17, 3300 AA Dordrecht, The Netherlands. www.springer.com

Printed on acid-free paper

All Rights Reserved © 2007 Springer No part of this work may be reproduced, stored in a retrieval system, or transmitted in any form or by any means, electronic, mechanical, photocopying, microfilming, recording or otherwise, without written permission from the Publisher, with the exception of any material supplied specifically for the purpose of being entered and executed on a computer system, for exclusive use by the purchaser of the work.

To my grandsons: Shachar, Eitan, and Sarel ¬ §¥¡£ §¥¡¦ ©´ ('¢ ±²® ,£¦³¨)

Contents

1 Notation and terminology

1

2 Fields

5

3 Vector spaces over a field

17

4 Algebras over a field

33

5 Linear independence and dimension

49

6 Linear transformations

79

7 The endomorphism algebra of a vector space

99

8 Representation of linear transformations by matrices

117

9 The algebra of square matrices

131

10 Systems of linear equations

169

11 Determinants

199

12 Eigenvalues and eigenvectors

229

13 Krylov subspaces

267 vii

viii

Contents

14 The dual space

285

15 Inner product spaces

299

16 Orthogonality

325

17 Selfadjoint Endomorphisms

349

18 Unitary and Normal endomorphisms

369

19 Moore-Penrose pseudoinverses

389

20 Bilinear transformations and forms

399

A Summary of Notation

423

Index

427

For whom is this book written?

Crow’s Law: Do not think what you want to think until you know what you ought to know.1

Linear algebra is a living, active branch of mathematical research which is central to almost all other areas of mathematics and which has important applications in all branches of the physical and social sciences and in engineering. However, in recent years the content of linear algebra courses required to complete an undergraduate degree in mathematics – and even more so in other areas – at all but the most dedicated universities, has been depleted to the extent that it falls far short of what is in fact needed for graduate study and research or for real-world application. This is true not only in the areas of theoretical work but also in the areas of computational matrix theory, which are becoming more and more important to the working researcher as personal computers become a common and powerful tool. Students are not only less able to formulate or even follow mathematical proofs, they are also less able to understand the underlying mathematics of the numerical algorithms they must use. The resulting knowledge gap has led to frustration and recrimination on the part of both students and faculty alike, with each silently – and sometimes not so silently – blaming the other for the resulting state of affairs. This book is written with the intention of bridging that gap. It was designed be used in one or more of several possible ways: (1) As a self-study guide; (2) As a textbook for a course in advanced linear algebra, either at the upper-class undergraduate level or at the first-year graduate level; or (3) As a reference book. It is also designed to be used to prepare for the linear algebra portion of prelim exams or PhD qualifying exams. This volume is self-contained to the extent that it does not assume any previous knowledge of formal linear algebra, though the reader is assumed to have been exposed, at least informally, to some basic ideas or techniques, such as matrix manipulation and the solution of a small system of linear equations. It does, however, assume a seriousness of purpose, considerable 1 This

law, attributed to John Crow of King’s College, London, is quoted by R. V. Jones in his book Most Secret War.

ix

x


motivation, and modicum of mathematical sophistication on the part of the reader. The book also contains a large number of exercises, many of which are quite challenging, which I have come across or thought up in over thirty years of teaching. Many of these exercises have appeared in print before, in such journals as American Mathematical Monthly, College Mathematics Journal, Mathematical Gazette, or Mathematics Magazine, in various mathematics competitions or circulated problem collections, or even on the internet. Some were donated to me by colleagues and even students, and some originated in files of old exams at various universities which I have visited in the course of my career. Since, over the years, I did not keep track of their sources, all I can do is offer a collective acknowledgement to all those to whom it is due. Good problem formulators, like the God of the abbot of Citeaux, know their own. Deliberately, difficult exercises are not marked with an asterisk or other symbol. Solving exercises is an integral part of learning mathematics and the reader is definitely expected to do so, especially when the book is used for self-study. Solving a problem using theoretical mathematics is often very different from solving it computationally, and so strong emphasis is placed on the interplay of theoretical and computational results. Real-life implementation of theoretical results is perpetually plagued by errors: errors in modelling, errors in data acquisition and recording, and errors in the computational process itself due to roundoff and truncation. There are further constraints imposed by limitations in time and memory available for computation. Thus the most elegant theoretical solution to a problem may not lead to the most efficient or useful method of solution in practice. While no reference is made to particular computer software, the concurrent use of a personal computer equipped symbolic-manipulation software such as Maple, Mathematica, Matlab or MuPad is definitely advised. In order to show the “human face” of mathematics, the book also includes a large number of thumbnail photographs of researchers who have contributed to the development of the material presented in this volume. Acknowledgements. Most of the first edition this book was written while the I was a visitor at the University of Iowa in Iowa City and at the University of California in Berkeley. I would like to thank both institutions for providing the facilities and, more importantly, the mathematical atmosphere which allowed me to concentrate on writing. This edition was extensively revised after I retired from teaching at the University of Haifa in April, 2004. I have talked to many students and faculty members about my plans for this book and have obtained valuable insights from them. In particular, I would like to acknowledge the aid of the following colleagues and students who were kind enough to read the preliminary versions of this book and


xi

offer their comments and corrections: Prof. Daniel Anderson (University of Iowa), Prof. Adi Ben-Israel (Rutgers University), Prof. Robert Cacioppo (Truman State University), Prof. Joseph Felsenstein (University of Washington), Prof. Ryan Skip Garibaldi (Emory University), Mr. George Kirkup (University of California, Berkeley), Prof. Earl Taft (Rutgers University), Mr. Gil Varnik (University of Haifa). Photo credits. The photograph of Dr. Shmuel Winograd is used with the kind permission of the Department of Computer Science of the City University of Hong Kong. The photographs of Prof. Ben-Israel, Prof. Blass, Prof. Kublanovskaya, and Prof. Strassen are used with their respective kind permissions. The photograph of Prof. Greville is used with the kind permission of Mrs. Greville. The photograph of Prof. Rutishauser is used with the kind permission of Prof. Walter Gander. The photograph of Prof. V. N. Faddeeva is used with the kind permission of Dr. Vera Simonova. The photograph of Prof. Zorn is used with the kind permission of his son, Jens Zorn. The photograph of J. W. Givens was taken from a group photograph of the participants at the 1964 Gatlinburg Conference on Numerical Algebra. All other photographs are taken from the MacTutor History of Mathematics Archive website (http://www-history.mcs.standrews.ac.uk/history/index.html), the portrait gallery of mathematicians at the Trucsmatheux website (http://trucsmaths.free.fr/), or similar websites. To the best knowledge of the managers of those sites, and to the best of my knowledge, they are in the public domain.

1 Notation and terminology

Sets will be denoted by braces, { } , between which we will either enumerate the elements of the set or give a rule for determining whether something is an element of the set or not, as in {x | p(x)}, which is read “the set of all x such that p(x)”. If a is an element of a set A we write a ∈ A; if it is not an element of A, we write a ∈ / A. When one enumerates the elements of a set, the order is not important. Thus {1, 2, 3, 4} and {4, 1, 3, 2} both denote the same set. However, we often do wish to impose an order on sets the elements of which we enumerate. Rather than introduce new and cumbersome notation to handle this, we will make the convention that when we enumerate the elements of a finite or countably-infinite set, we will assume an implied order, reading from left to right. Thus, the implied order on the set {1, 2, 3, . . .} is indeed the usual one. The empty set, namely the set having no elements, is denoted by ∅. Sometimes we will use the word “collection” as a synonym for “set”, generally to avoid talking about “sets of sets”. A finite or countably-infinite selection of elements of a set A is a list. Members of a list are assumed to be in a definite order, given by their indices or by the implied order of reading from left to right. Lists are usually written without brackets: a1 , . . . , an , though, in certain contexts, it will be more convenient to write them as ordered n-tuples (a1 , . . . , an ). Note that the elements of a list need not be distinct: 3, 1, 4, 1, 5, 9 is a list of six positive integers, the second and fourth elements of which are equal to 1. A countably-infinite list of elements of a set A is also often called 1

2

1. Notation and terminology

a sequence of elements of A. The set of all distinct members of a list is called the underlying subset of the list. If A and B are sets, then their union A ∪ B is the set of all elements that belong to either A or B, and their intersection A ∩ B is the set of all elements belonging both to A and to B. More generally, if {Ai | i ∈ Ω} is a (possibly-infinite) collection of sets, then i∈Ω Ai is the set of all elements that belong to at least one of the Ai and i∈Ω Ai is the set of all elements that belong to all of the Ai . If A and B are sets, then the difference set A B is the set of all elements of A which do not belong to B. A function f from a nonempty set A to a nonempty set B is a rule which assigns to each element a of A a unique element f (a) of B. The set A is called the domain of the function and the set B is called the range of the function. To denote that f is a function from A to B, we write f : A → B. To denote that an element b of B is assigned to an element a of A by f, we write f : a → b. (Note the different form of the arrow!) This notation is particularly helpful in the case that the function f is defined by a formula. Thus, for example, if f is a function from the set of integers to the set of integers defined by f : a → a3 , then we know that f assigns to each integer its cube. The set of all functions from a nonempty set A to a nonempty set B is denoted by B A . If f ∈ B A and if A is a nonempty subset of A, then the restriction of f to A is the function f : A → B defined by f : a → f (a ) for all a ∈ A . Functions f and g in B A are equal if and only if f (a) = g(a) for all a ∈ A. In this case we write f = g. A function f ∈ B A is monic if and only if it assigns different elements of B to different elements of A, i.e. if and only if f (a1 ) = f (a2 ) whenever a1 = a2 in A. A function f ∈ B A is epic if and only if every element of B is assigned by f to some element of A. A function which is both monic and epic is bijective. A bijective function from a set A to a set B determines a bijective correspondence between the elements of A and the elements of B. If f : A → B is a bijective function, then we can define the inverse function f −1 : B → A defined by the condition that f −1 (b) = a if and only if f (a) = b. This inverse function is also bijective. A bijective function from a set A to itself is a permutation of A. Note that there is always at least one permutation of any nonempty set A, namely the identity function a → a. The cartesian product A1 × A2 of nonempty sets A1 and A2 is the set of all ordered pairs (a1 , a2 ), where a1 ∈ A1 and a2 ∈ A2 . More generally, if A1 , . . . , An is a list of nonempty sets, then A1 × . . . × An is the set of all ordered n-tuples (a1 , . . . , an ) satisfying the condition that ai ∈ Ai for each 1 ≤ i ≤ n. Note that each ordered n-tuple (a1 , . . . , an )

1. Notation and terminology

3

uniquely defines a function f : {1, . . . , n} → ∪ni=1 Ai given by f : i → ai n for each 1 ≤ i ≤ n. Conversely, each function f : {1, . . . , n} → i=1 Ai satisfying the condition that f (i) ∈ Ai for 1 ≤ i ≤ n, defines such an ordered n-tuple, namely (f (1), . . . , f (n)). This suggests a method for defining the cartesian product of an arbitrary collection of nonempty sets. If {Ai | i ∈ Ω} is an arbitrary collection of nonempty sets, then the set i∈Ω Ai is defined to be the set of all those functions f from Ω to i∈Ω Ai satisfying the condition that f (i) ∈ Ai for each i ∈ Ω. The existence of such functions is guaranteed by a fundamental axiom of set theory, known as the Axiom of Choice. A certain amount of controversy surrounds this axiom, and there are mathematicians who prefer to make as little use of it as possible. However, we will need it constantly throughout this book, and so will always assume that it holds. In the foregoing construction we did not assume that the sets Ai were necessarily distinct. Indeed, it may very well happen that there exists a set A such that Ai = A for all i ∈ Ω. In that case, we see that i∈Ω Ai is just AΩ . If the set Ω is finite, say Ω = {1, . . . , n}, then we write An instead of AΩ . Thus, An is just the set of all ordered n-tuples (a1 , . . . , an ) of elements of A. We use the following standard notation for some common sets of numbers N Z Q R C

the the the the the

set set set set set

of of of of of

all all all all all

nonnegative integers integers rational numbers real numbers complex numbers

Other notion is introduced throughout the text, as is appropriate. See the Summary of Notation at the end of the book.

2 Fields

The way of mathematical thought is twofold: the mathematician first proceeds inductively from the particular to the general and then deductively from the general to the particular. Moreover, throughout its development, mathematics has shown two aspects – the conceptual and the computational – the symphonic interleaving of which forms one of the major aspects of the subject’s aesthetic. Let us therefore begin with the first mathematical structure: numbers. By the Hellenistic times, mathematicians distinguished between two types of numbers: the rational numbers, namely those which could be written in the form m n for some integer m and some nonnegative integer n, and those numbers representing the geometric magnitude of segments of the line, which today we call real numbers and which, in decimal notation, are written in the form m.k1 k2 k3 . . . where m is an integer and the ki are digits. The fact that the set Q of rational numbers is not equal to the set R of real numbers was already noticed by the followers of the mathematician/mystic Pythagoras. On both sets of numbers we define operations of addition and multiplication which satisfy certain rules of manipulation. Isolating these rules as part of a formal system was a task first taken on in earnest by nineteenth-century British and German mathematicians. From their studies evolved the notion of a field, which will be basic to our considerations. However, since fields are not our primary object of study, we will 5

6

2. Fields

delve only minimally into this fascinating notion. A serious consideration of field theory must be deferred to an advanced course in abstract algebra.1 A nonempty set F together with two functions F ×F → F , respectively called addition (as usual, denoted by +) and multiplication (as usual, denoted by · or by concatenation), is a field if the following conditions are satisfied: (1) (associativity of addition and multiplication): a + (b + c) = (a + b) + c and a(bc) = (ab)c for all a, b, c ∈ F . (2) (commutativity of addition and multiplication): a + b = b + a and ab = ba for all a, b ∈ F. (3) (distributivity of multiplication over addition): a(b + c) = ab + ac for all a, b, c ∈ F . (4) (existence of identity elements for addition and multiplication): There exist distinct elements of F , which we will denote by 0 and 1 respectively, satisfying a + 0 = a and a1 = a for all a ∈ F . (5) (existence of additive inverses): For each a ∈ F there exists an element of F , which we will denote by −a, satisfying a + (−a) = 0. (6) (existence of multiplicative inverses): For each 0 = a ∈ F there exists an element of F , which we will denote by a−1 , satisfying a−1 a = 1. Note that we did not assume that the elements −a and a−1 are unique, though we will soon prove that in fact they are. If a and b are elements of a field F , we will follow the usual conventions by writing a − b instead of a + (−b) and ab instead of ab−1 . Moreover, if 0 = a ∈ F and if n is a positive integer, then na denotes the sum a + . . . + a (n summands) and an denotes the product a · . . . · a (n factors). If n is a negative integer, then na denotes (−n)(−a) and an denotes (a−1 )−n . Finally, if n = 0 then na denotes the field element 0 and an denotes the field element 1. For 0 = a ∈ F , we define na = 0 for all integers n and

1

The development of the abstract theory of fields is generally credited to the 19thcentury German mathematician Heinrich Weber, based on earlier work by the German mathematicians Richard Dedekind and Leopold Kronecker. Another 19th-century mathematician, the British Augustus De Morgan, was the first to isolate the importance of such properties as associativity, distributivity, and so forth. The final axioms of a field are due to the 20th-century German mathematician Ernst Steinitz.

2. Fields

7

an = 0 for all positive integers n. The symbol 0k is not defined for k ≤ 0. As an immediate consequence of the associativity and commutativity of addition, we see that the sum of any list a1 , . . . , an of elements of a field F is the same, no matter in which order we add them. We can therefore unambiguously write a1 + . . . + an . This sum is also often denoted by n a . Similarly, the product of these elements is the same, no matter i i=1 in which order we multiply them. We can therefore nunambiguously write a1 · . . . · an . This product is also often denoted by i=1 ai . Also, a simple inductive argument shows that multiplication distributes overarbitrary n sums: n if a ∈ F and b1 , . . . bn is a list of elements of F then a ( i=1 bi ) = i=1 abi . We easily see that Q and R, with the usual addition and multiplication, are fields. A subset G of a field F is a subfield if and only if it contains 0 and 1, is closed under addition and multiplication, and contains the additive and multiplicative inverses of all of its nonzero elements. Thus, for example, Q is a subfield of R. The intersection of a collection of subfields of a field F is again a subfield of F. We now want to look at several additional important examples of fields. Example: Let C = R2 and define operations of addition and multiplication on C by setting (a, b) + (c, d) = (a + c, b + d) and (a, b) · (c, d) = (ac − bd, ad + bc). These operations define the structure of a field on C, in which the identity element for addition is (0, 0), the identity element for multiplication is (1, 0), the additive inverse of (a, b) is (−a, −b), and a −b −1 , (a, b) = a2 + b2 a2 + b2 for all (0, 0) = (a, b). This field is called the field of complex numbers. The set of all elements of C of the form (a, 0) forms a subfield of C, which we normally identify with R and therefore it is standard to consider R as a subfield of C. In particular, we write a instead of (a, 0) for any real number a. The element (0, 1) of C is denoted by i. This 2 element √ satisfies the condition that i = (−1, 0) and so it is often written −1. We also note that any element (a, b) of C can be written as as (a, 0) + b(0, 1) = a + bi, and, indeed, that is the way complex numbers are usually written and how we will denote them from now on. If z = a + bi, then a is the real part of z, which is often denoted by Re(z), while bi is the imaginary part of z, which is often denoted by Im(z). The

8

2. Fields

field of complex numbers is extremely important in mathematics. From a geometric point of view, if we identify R with the set of points on the Euclidean line, as one does in analytic geometry, then it is natural to identify C with the set of points in the Euclidean plane.2 If z = a + bi ∈ C then we denote the complex number a − bi, called the complex conjugate of z, by z. It is easy to see3 that for all z, z ∈ C we have z + z = z + z , −z = −z, zz = z · z , z −1 = (z)−1 , and z = z. The number zz equals a2 + b2 , which is a nonnegative real number and so has a square root in R, which we will denote by |z|. Note that |z| is nonzero whenever z = 0. From a geometric point of view, this number is just the distance from the number z, considered as a point in the euclidean plane, to the origin, just as the usual absolute value |a| of a real number a is the distance between a and 0 on the real line. It is easy to see that if y and z are complex numbers then |yz| = |y| · |z| and |y + z| ≤ |y| + |z|. Moreover, if z = a + bi then √ z + z = 2a ≤ 2|a| = 2 a2 ≤ 2 a2 + b2 = 2|z|. We also note, as a direct consequence of the definition, that |z| = |z| for every complex number z and so z −1 = |z|−2 z for all 0 = z ∈ C. Example: The set Q2 is a subfield of the field C defined above. However, it is also possible to define field structures on Q2 in other ways. Indeed, let F = Q2 and let p be a fixed prime integer. Define addition and multiplication on F by setting (a, b) + (c, d) = (a + c, b + d) and (a, b) · (c, d) = (ac + bdp, ad + bc). Again, one can check that F is indeed a field and that, again, the set of all elements of F of the form (a, 0) is a subfield, which we will identify with Q. Moreover, the additive inverse of (a, b) ∈ F is (−a, −b) and

2 The term “imaginary” was coined by the 17thcentury√French philosopher and mathematician Ren´ e Descartes. The use of i to denote −1 was introduced by 18th-century Swiss mathematician Leonhard Euler. The geometric representation of the complex numbers was first proposed at the end of the 18th century by the Norwegan surveyor Caspar Wessel, and later by the French accountant Jean-Robert Argand. 3 When a mathematician says that something is “easy to see” or “trivial”, it means that you are expected to take out a pencil and paper and spend some time – often considerable – checking it out by yourself.

2. Fields

9

the multiplicative inverse of (0, 0) = (a, b) ∈ F is

a −b , a2 − pb2 a2 − pb2

.

√ (We note that a2 −pb2 is the product of the nonzero real numbers a+b p √ and a − b p and so is nonzero.) The element (0, 1) of F satisfies √ (0, 1)2 = (p, 0) and so one usually denotes it by p and, as before, any √ element of F can be written in the form √ a + b p, where a, b ∈ Q. The field F is usually denoted by Q p . Since there are infinitelymany distinct prime integers, we see that there are infinitely-many ways of defining different field structures on Q × Q, all having the same addition. Example: Fields do not have to be infinite. Let p be a positive integer and let Z/(p) = {0, 1, . . . , p − 1}. For each nonnegative integer n, let us, for the purposes of this example, denote the remainder after dividing n by p as [n]p . Thus we note that [n]p ∈ Z/(p) for each nonnegative integer n and that [i]p = i for all i ∈ Z/(p). We now define operations on Z/(p) by setting [n]p + [k]p = [n + k]p and [n]p · [k]p = [nk]p . It is easy to check that if the integer p is prime then Z/(p), together with these two operations, is again a field, known as the Galois4 field of order p. This field is usually denoted by GF (p). While Galois fields were first considered mathematical curiosities, they have since found important applications in coding theory, cryptography, and modeling of computer processes. These are not the only possible finite fields. Indeed, it is possible to show that for each prime integer p and each positive integer n there exists an (essentially unique) field with pn elements, usually denoted by GF (pn ). Example: Some important structures are “very nearly” fields. For example, let R∞ = R ∪ {∞}, and define operations and on R∞ by setting   min{a, b} if a, b ∈ R b if a = ∞ ab=  a if b = ∞

4

The 19th-century French mathematical genius Evariste Galois, who died at the age of 21, was the first to consider such structures. The study of finite and infinite fields was unified in the 1890’s by Eliakim Hastings Moore, the first American-born mathematician to achieve an international reputation.

10

2. Fields

and ab=

a + b if a, b ∈ R . ∞ otherwise

This structure, called the optimization algebra, satisfies all of the conditions of a field except for the existence of additive inverses (such structures are known as semifields). As the name suggests, it has important applications in optimization theory and the analysis of discrete-event dynamical systems. There are several other semifields which have important applications and which have been extensively studied. Another possibility of generalizing the notion of a field is to consider an algebraic structure which satisfies all of the conditions of a field except for the existence of multiplicative inverses, and to replace that condition by the condition that if a, b = 0 then ab = 0. Such structures are known as integral domains. The set Z of all integers is the simplest example of an integral domain which is not a field. Algebras of polynomials over a field, which we will consider later, are also integral domains. In a course in abstract algebra, one proves that any integral domain can be embedded in a field. In the field GF (p) which we defined above, one can easily see that the sum 1 + . . . + 1 (p summands) equals 0. On the other hand, in the field Q, the sum of any number of copies of 1 is always nonzero. This is an important distinction which we will need to take into account in dealing with structures over fields. We therefore define the characteristic of a field F to be equal to the smallest positive integer p such that 1 + . . . + 1 (p summands) equals 0 – if such an integer p exists – and to be equal to 0 otherwise. We will not delve deeply into this concept, which is dealt with in courses on field theory, except to note that the characteristic of a field, if nonzero, always turns out to be a prime number. In the definition of a field, we posited the existence of distinct identity elements for addition and multiplication, but did not claim that these elements were unique. It is, however, very easy to prove that fact. (2.1) Proposition: Let F be a field. (1) If e is an element of F satisfying e + a = a for all a ∈ F then e = 0; (2) If u is an element of F satisfying ua = a for all a ∈ F then u = 1.

Proof: By definition we note that e = e + 0 = 0 and u = u1 = 1.

2. Fields

11

Similarly, we prove that additive and multiplicative inverses, when they exist, are unique. Indeed, we can prove a stronger result. (2.2) Proposition: If a and b are elements of a field F then: (1) There exists a unique element c of F satisfying a + c = b. (2) If a = 0 then there exists a unique element d of F satisfying ad = b. Proof: (1) Choose c = b − a. Then a + c = a + (b − a) = a + [b + (−a)] = a + [(−a) + b] = [a + (−a)] + b = 0 + b = b. Moreover, if a + x = b then x

= 0 + x = [(−a) + a] + x = (−a) + (a + x) = (−a) + b = b − a,

proving uniqueness. (2) Choose d = a−1 b. Then ad = a(a−1 b) = (aa−1 )b = 1b = b. Moreover, if ay = b then y = 1y = (a−1 a)y = a−1 (ay) = a−1 b, proving uniqueness. We now summarize some of the elementary properties of fields, which are all we will need for our discussion. (2.3) Proposition: If a, b, and c are elements of a field F then: (1) 0a = 0; (2) (−1)a = −a; (3) a(−b) = −(ab) = (−a)b; (4) −(−a) = a; (5) (−a)(−b) = ab; (6) −(a + b) = (−a) + (−b); (7) a(b − c) = ab − ac; −1 = a; (8) If a = 0 then a−1 (9) If a, b = 0 then (ab)−1 = b−1 a−1 ; (10) If a + c = b + c then a = b; (11) If c = 0 and ac = bc then a = b. (12) If ab = 0 then a = b or b = 0. Proof: (1) Since 0a + 0a = (0 + 0)a = 0a, we can add −(0a) to both sides of the equation to obtain 0a = 0. (2) Since (−1)a + a = (−1)a + 1a = [(−1) + 1]a = 0a = 0 and also (−a) + a = 0, we see from Proposition 2.2 that (−1)a = −a.

12

2. Fields

(3) By (2) we have a(−b) = a[(−1)b] = (−1)ab = −(ab) and similarly (−a)b = −(ab). (4) Since a + (−a) = 0 = −(−a) + (−a), this follows from Proposition 2.2. (5) From (3) and (4) it follows that (−a)(−b) = a[−(−b)] = ab. (6) Since (a + b) + [(−a) + (−b)] = a + b + (−a) + (−b) = 0 and (a + b) + [−(a + b)] = 0, the result follows from Proposition 2.2. (7) By (3) we have a(b − c) = ab + a(−c) = ab + [−(ac)] = ab − ac. −1 −1 a = 1 = aa−1 , this follows from Proposition (8) Since a−1 2.2. (9) Since a−1 b−1 (ba) = a−1 ab−1 b = 1 = (ab)−1 (ba), the result follows from Proposition 2.2. (10) This is an immediate consequence of adding −c to both sides of the equation. (11) This is an immediate consequence of multiplying both sides of the equation by c−1 . (12) If b = 0 we are done. If b = 0 then by (1) it follows that multiplying both sides of the equation by b−1 will yield a = 0. (2.4) Proposition: Let a be a nonzero element of a finite field F having q elements. Then a−1 = aq−2 . Proof: If q = 2 then F = GF (2) and a = 1, so the result is immediate. Hence we can assume q > 2. Let B = {a1 , . . . aq−1 } be the nonzero elements of F, written in some arbitrary order. Then aai = aah for i = h since, were they equal, we would have ai = a−1 (aai ) = a−1 (aah ) = ah . Therefore B = {aa1 , . . . aaq−1 } and so q−1 i=1

ai =

q−1

(aai ) = aq−1

i=1

q−1

ai .

i=1

Moreover, this is a product of nonzero elements of F and so, by Proposition 2.3(12), is also nonzero. Therefore, by Proposition 2.3(11), 1 = aq−1 and so aa−1 = 1 = aq−1 = a(aq−2 ), implying that a−1 = aq−2 .

Exercises Exercise 1 Let F be a field and let G = F × F. Define operations of addition and multiplication on G by setting (a, b) + (c, d) = (a + c, b + d) and (a, b) · (c, d) = (ac, bd). Do these operations define the structure of a field on G?

2. Fields

13

Exercise 2 Let r ∈ R and let 0 = s ∈ R. Define operations and on R × R by setting (a, b) (c, d) = (a + c, b + d) and (a, b) (c, d) = (ac − bd(r2 + s2 ), ad + bc + 2rbd). Do these operations, considered as addition and multiplication respectively, define the structure of a field on R × R? Exercise 3 Define a new operation † on R by setting a † b = a3 b. Show that R, on which we have the usual addition and this new operation as multiplication, satisfies all of the axioms of a field with the exception of one. Exercise 4 Let 1 < t ∈ R and let F = {a ∈ R | a < 1}. Define operations ⊕ and on F as follows: (1) a ⊕ b = a + b − ab for all a, b ∈ F ; (2) a b = 1 − tlogt (1−a) logt (1−b) for all a, b ∈ F. For which values of t does F, together with these operations, form a field? √ Exercise √ 5 Show that the set of all real numbers of the form a + b 2 + √ c 3 + d 6, where a, b, c, d ∈ Q, forms a subfield of R. √ Exercise 6 Is {a + b 15 | a, b ∈ Q} a subfield of R? Exercise 7 Show that the field R has infinitely-many distinct subfields. Exercise 8 Let F be a field and define a new operation ∗ on F by setting a ∗ b = a + b + ab. When is (F, +, ∗) a field? Exercise 9 Let F be a field and let Gn be the subset of F consisting of all elements which can be written as a sum of n squares of elements of F. (1) Is the product of two elements of G2 again an element of G2 ? (2) Is the product of two elements of G4 again an element of G4 ? √ Exercise 10 Let t = 3 2 ∈ R and let S be the set of all real numbers of the form a + bt + ct2 , where a, b, c ∈ Q. Is S a subfield of R? Exercise 11 Let F be a field. Show that the function a → a−1 is a permutation of F {0F }. Exercise 12 Show that every z ∈ C satisfies z 4 + 4 = (z − 1 − i)(z − i + i)(z + 1 + i)(z + 1 − i). Exercise 13 In each of the following, find the set of all complex numbers z = a + bi satisfying the given relation. Note that this set may be empty or may be all of C. Justify your result in each case.

14

2. Fields

(a) (b) (c) (d) (e)

√ z 2 = 1 (1 + i 3); √ 2 2 |z| ≥ |a| + |b|; |z| + z = √ 2 + i; 12 i; z4 = 2 − z 4 = −4.

Exercise 14 Let y be a complex number satisfying |y| < 1. Find the set of all complex numbers z satisfying |z − y| ≤ |1 − yz|. Exercise 15 Let z1 , z2 , and z3 be complex numbers satisfying the condition that |zi | = 1 for i = 1, 2, 3. Show that |z1 z2 + z1 z3 + z2 z3 | = |z1 + z2 + z3 |. Exercise 16 For any z1 , z2 ∈ C, show that |z1 |2 + |z2 |2 − z1 z2 − z1 z2 = |z1 − z2 |2 . 2

Exercise 17 Show that |z + 1| ≤ |z + 1| + |z| for all z ∈ C. Exercise 18 If z ∈ C, find w ∈ C satisfying w2 = z. Exercise 19 Define new operations ◦ and on C by setting y◦z = |y|z and

0 if y = 0 yz = 1 yz otherwise |y| for all y, z ∈ C. Is it true that w (y ◦ z) = (w y) ◦ (w z) and w ◦ (y z) = (w ◦ y) (w ◦ z) for all w, y, z ∈ C? Exercise 20 Let 0 = z ∈ C. Show that there are infinitely-many complex numbers y satisfying the condition yy = zz. Exercise 21 (Abel’s inequality5 ): Let z1 , . . . , zn be a list of complex k numbers and, for each 1 ≤ k ≤ n, let sk = i=1 zi . For real numbers a1 , . . . , an satisfying a1 ≥ a2 ≥ . . . ≥ an ≥ 0, show that n ai zi ≤ a1 max |sk | . 1≤k≤n i=1

5

Nineteenth-century Norwegian mathematicial genius Niels Henrik Abel died tragically at the age of 26.

2. Fields

15

Exercise 22 Let 0 = z0 ∈ C satisfy the condition |z0 | < 2. Show that there are precisely two complex numbers, z1 and z2 , satisfying |z1 | + |z2 | = 1 and z1 + z2 = z0 . Exercise 23 If p is a prime positive integer, find all subfields of GF (p). √ Exercise 24 Find elements c, d = ±1 in the field Q 5 satisfying cd = 19. Exercise 25 Let F be the set of all real numbers of the form √ √ 2 3 3 a+b 5 +c 5 , where a, b, c ∈ Q. Is F a subfield of R? Exercise 26 Let p be a prime positive integer and let a ∈ GF (p). Does there necessarily exist an element b of GF (p) satisfying b2 = a? Exercise 27 Let F = GF (11) and let G = F × F. Define operations of addition and multiplication on G by setting (a, b) + (c, d) = (a + c, b + d) and (a, b) · (c, d) = (ac + 7bd, ad + bc). Do these operations define the structure of a field on G? Exercise 28 Let F be a field and let G be a finite subset of F {0} containing 1 and satisfying the condition that if a, b ∈ F then ab−1 ∈ G. Show that there exists an element c ∈ G such that G = {ci | i ≥ 0}. Exercise 29 Let F be a field satisfying the condition that the function a → a2 is a permutation of F. What is the characteristic of F ? Exercise 30 Is Z/(6) an integral domain? √ √ Exercise 31 Let F = {a + b 5 ∈ Q( 5) | a, b ∈ Z}. Is F an integral domain? Exercise 32 Let F be an integral domain and let a ∈ F satisfy a2 = a. Show that a = 0 or a = 1. Exercise 33 Let a be a nonzero element in an integral domain F. If b = c are distinct elements of F, show that ab = ac. Exercise 34 Let F be an integral domain and let G be a nonempty subset of F containing 0 and 1 and closed under the operations of addition and multiplication in F . Is G necessarily an integral domain? Exercise 35 Let U be the set of all positive integers and let F be the set of all functions from U to C. Define operations of addition and multiplication on F by setting f + g : k → f (k) + g(k) and f g : k → ij=k f (i)g(j) for all k ∈ U. Is F, together with these operations, an integral domain? Is it a field?

16

2. Fields

Exercise 36 Let F be the set of all functions f from R to itself n of the form f : t → k=1 [ak cos(kt) + bk sin(kt)] , where the ak and bk are real numbers and n is some positive integer. Define addition and multiplication on F by setting f +g : t → f (t)+g(t) and f g : t → f (t)g(t) for all t ∈ R. Is F, together with these operations, an integral domain? Is it a field? Exercise 37 Show that every integral domain having only finitely-many elements is a field. Exercise 38 Let F be a field of characteristic other than 2 in which n 2 a there exist elements a1 , . . . , an satisfying i=1 i = −1. (This happens, for example, in the case F = C). Show that for any c ∈ F there exist k elements b1 , . . . , bk of F satisfying c = i=1 b2i . Exercise 39 Let p be a prime integer. Show that for each a ∈ GF (p) there exist elements b and c of GF (p), not necessarily distinct, satisfying a = b2 + c2 . Exercise 40 Let F be a field in which we have elements a, b, and c (not necessarily distinct) satisfying a2 +b2 +c2 = −1. Show that there exist (not necessarily distinct) elements d and e of F, satisfying d2 +e2 = −1. Exercise 41 Is every nonzero element of the field GF (5) in the form 2i for some positive integer i? What happens in the case of the field GF (7)? Exercise 42 Find the set of all fields F in which there exists an element a satisfying the condition that a + b = a for all b ∈ F {a}. Exercise 43 (Binomial Formula) If a and b are elements n of a field F, and if n is a positive integer, show that (a + b)n = k=0 nk ak bn−k . Exercise 44 Let F be a field of characteristic p > 0. Use the previous two exercises to show that the function γ : F → F defined by γ : a −→ ap is monic. Exercise 45 Let a and b be nonzero elements of a finite field F, and let m and n be positive integers satisfying am = bn = 1. Show that there exists a nonzero element c of F satisfying ck = 1, where k is the least common multiple of m and n. Exercise 46 If a is a nonzero element of a field F, show that (−a)−1 = −(a−1 ). Exercise 47 A field F is orderable if and only if there exists a subset P closed under addition and multiplication such that for each a ∈ F precisely one of the following conditions holds: (i) a = 0; (ii) a ∈ P ; (iii) −a ∈ P. Show that GF (5) is not orderable.

3 Vector spaces over a field

If n > 1 is an integer and if F is a field, it is natural to define addition on the set F n componentwise: (a1 , . . . , an ) + (b1 , . . . , bn ) = (a1 + b1 , . . . , an + bn ). More generally, if Ω is any nonempty set and if F Ω is the set of all functions from Ω to the field F, we can define addition on F Ω by setting f + g : i → f (i) + g(i) for each i ∈ Ω. Given these definitions, is it possible to define multiplication in such a manner that F n or F Ω will become a field naturally containing F as a subfield? We have seen that if n = 2 and if F = R or F = Q, this is possible – and, indeed, in the latter case there are several different methods of doing it. If F = GF (p) then it is possible to define such a field structure on F n for every integer n > 1. However in general the answer is negative – as we will show in a later chapter for the specific case of Rk , where k > 2 is an odd integer. Nonetheless, it is possible to construct another important and useful structure on these sets, and this structure will be the focus of our attention for the rest of this book. We will first give the formal definition, and then look at a large number of examples. Let F be a field. A nonempty set V, together with a function V × V → V called vector addition (denoted, as usual, by +) and a function F × V → V called scalar multiplication (denoted, as a rule, 17

18

3. Vector spaces over a field

by concatenation) is a vector space over F if the following conditions are satisfied: (1) (associativity of vector addition): v + (w + y) = (v + w) + y for all v, w, y ∈ V. (2) (commutativity of vector addition): v + w = w + v for all v, w ∈ V. (3) (existence of a identity element for vector addition): There exists an element 0V of V satisfying the condition that v + 0V = v for all v ∈ V. (4) (existence of additive inverses): For each v ∈ V there exists an element of V, which we will denote by −v, which satisfies v +(−v) = 0V . (5) (distributivity of scalar multiplication over vector addition and of scalar multiplication over field addition): a(v + w) = av + aw and (a + b)v = av + bv for all a, b ∈ F and v, w ∈ V. (6) (associativity of scalar multiplication): (ab)v = a(bv) for all a, b ∈ F and v ∈ V. (7) (existence of identity element for scalar multiplication): 1v = v for all v ∈ V. The elements of V are called vectors and the elements of F are called scalars1 . Example: Note that condition (7), apparently trivial, does not follow from the other conditions. Indeed, if we take V = F but define scalar multiplication by av = 0V for all a ∈ F and v ∈ V, we would get a structure which satisfies conditions (1) - (6) but not condition (7). If v, w ∈ V we again write v − w instead of v + (−w). As we noted when we talked about fields, if v1 , . . . , vn is a list of vectors in a vector space V over a field F, the associativity of vector addition allows us to unambiguously write v1 + . . . + vn , and this sum is often n denoted by i=1 nvi . Moreover, if a ∈ F is a scalar then we surely have n a ( i=1 vi ) = ( i=1 avi ) . Similarly, if a1 , . . . , an is a list of scalars and

1

The theory of vector spaces was developed in the 1880’s by the American engineer and physicist, Josiah Willard Gibbs and the British engineer Oliver Heaviside, based on the work of the Scottish physicist James Clerk Maxwell, the German high-school teacher Herman Grassmann, and the French engineer Jean Claude Saint-Venant.


19

n n if v ∈ V, then we have ( i=1 ai ) v = i=1 ai v. We will also adopt the convention that the sum of an empty set of vectors is equal to 0V . Clearly any field F is a vector space over itself, where we take the vector addition to be the addition in F and scalar multiplication to be the multiplication in F. We also note an extremely important construction. Let F be a field and let Ω be a nonempty set. Assume that, for each i ∈ Ω, we are given a vector space Vi over F, the addition in which we will denote by +i (the vector spaces Vi need not, however, be distinct from one another).Recall that i∈Ω Vi is the set of all those functions f from Ω to i∈Ω Vi which satisfy the condition that f (i) ∈ V for each i ∈ Ω. We now define i the structure of a vector space on i∈Ω Vi as follows: if f, g ∈ i∈Ω Vi then f + g is the function in V given by f + g : i → f (i) + i g(i) i∈Ω i for each i ∈Ω. Moreover, if a ∈ F and f ∈ i∈Ω Vi , then af is the function in i∈Ω Vi given by af : i → a [f (i)] for each i ∈ Ω. It is routine to verify that all of the axioms of a vector space are satisfied in this case. For example, the identity element for vector addition is just the function in i∈Ω Vi given by i → 0Vi for each i ∈ Ω. This vector space is called the is finite, direct product of the vector spaces Vi over F. If the set Ω say Ω = {1, . . . , n}, then we often write V1 × . . . × Vn instead of i∈Ω Vi . If all of the vector spaces Vi are equal to the same vector space V, then n we write V Ω instead of i∈Ω Vi and if Ω = {1, . . . , n} we write V Ω instead of V . Note that a function f from a finite set Ω = {1, . . . , n} to a vector space V is totally defined by the list f (1), f (2), . . . , f (n) of its values. Conversely, any list v1 , . . . , vn of elements of V uniquely defines such a function f given by f : i → vi . Therefore this notation agrees with our previous use of the symbol V n to denote sets of n-tuples of elements of V. However, to emphasize the vector space structure here, we   v1   will write the elements of V n as columns of the form  ...  , where the vn vi are (not necessarily distinct) elements of V. Usually, we will consider the case V = F. Vector addition and scalar multiplication in V n are then defined by the rules           v1 w1 v1 + w1 v1 cv1   ..   ..    .   .  ..  and c  ..  =  ..  .  . + . = . vn

wn

vn + wn

vn

cvn

The “classical” study of vector spaces centers around the spaces Rn , the vectors in which are identified with the points in n-dim ensional euclidean

20


space2 . However, other vector spaces also have important applications. Vector spaces of the form Cn are needed for the study of functions of several complex variables. In algebraic coding theory, one is interested in spaces of the form F n , where F is a finite field. The vectors in this space are words of length n and the field F is the alphabet in which these words are written. Thus, for example, a popular choice for F is the Galois field GF (28 ), the 256 elements of which are identified with the 256 ASCII symbols. Let V be a vector space, let k and n be positive integers, and let Ω = {(i, j) | 1 ≤ i ≤ k, 1 ≤ j ≤ n}. There exists a bijective correspondence between V Ω and the set of all rectangular arrays of the   v11 . . . v1n  ..  in which the entries v form  ... ij are elements of V. .  vk1

...

vkn

Such an array is called a k × n matrix3 over V. We will denote the set of all such matrices by Mk×n (V ). Addition and scalar multiplication in Mk×n (V ) is given by     v11 . . . v1n w11 . . . w1n  .. ..  +  .. ..   . .   . .    = 

vk1

...

vkn

v11 + w11 .. .

...

vk1 + wk1

...

wk1

... 

wkn

v1n + w1n  ..  . vkn + wkn

2 The first explicit statement of the geometric “parallelogram law” for adding vectors in R2 was given by the sixteenth-century Pisan scientist Galileo Galilei.

3 The term “matrix” was first coined by the 19th-century British mathematician James Joseph Sylvester in 1848. Sylvester was one of the major researchers in the theory of matrices and determinants.




 cv1n ..  . The identity element .  ... . . . cvkn   0V . . . 0V  ..  . for vector addition in Mk×n (V ) is the 0-matrix O =  ... .  0V . . . 0V Note that V n = Mn×1 (V ).

v11  and c  ... vk1

...

  v1n cv11 ..  =  .. .   . cvk1 vkn

21

...

If V is a vector space and if Ω = N, then the elements of V Ω are infinite sequences [v0 , v1 , . . .] of elements of V. We will denote this vector space, which we will need later, by V ∞ . Again, the space of particular interest will be F ∞ . Example: If F is a subfield of a field K, then K is a vector space over F, with addition and multiplication just being the operations in K. Thus, in particular, we can think of C as a vector space over R and of R as a vector space over Q. Example: Let A be a nonempty set and let V be the collection of all subsets of A. Let us define addition of elements of V as follows: if B and C are elements of V then B +C = (B ∪C)(B ∩C). This operation is usually called the symmetric difference of B and C. This definition turns V into a vector space over GF (2), where scalar multiplication is defined by 0B = ∅ and 1B = B for all B ∈ V. This is actually just a special case of what we have seen before. Indeed, we note that there is a bijective function from V to GF (2)A which assigns to each subset B of A its characteristic function, namely the function χB defined by

1 if a ∈ B χB : a → 0 otherwise and it is easy to see that χA + χB = χA+B , while χA χB = χA∩B . (3.1) Proposition: Let V be a vector space over a field F . (1) If z ∈ V satisfies z + v = v for all v ∈ V then z = 0V . (2) If v, w ∈ V then there exists a unique element y ∈ V satisfying v + y = w.

Proof: The proof is similar to the proofs of Proposition 2.1(1) and Proposition 2.2(1). (3.2) Proposition: Let V be a vector space over a field F . If v, w ∈ V and if a ∈ F, then:

22


(1) (2) (3) (4) (5) (6) (7) (8) (9)

a0V = 0V ; 0v = 0V ; (−1)v = −v; (−a)v = −(av) = a(−v); −(−v) = v; av = (−a)(−v); −(v + w) = −v − w; a(v − w) = av − aw; If av = 0V then either v = 0V or a = 0.

Proof: The proof is similar to the proof of Proposition 2.3.

Let V be a vector space over a field F . A nonempty subset W of V is a subspace of V if and only if it is a vector space in its own right with respect to the addition and scalar multiplication defined on V. Thus, any vector space V is a subspace of itself, called the improper subspace; any other subspace is proper. Also, {0V } is surely a subspace of V, called the trivial subspace; any other subspace is nontrivial. Note that the two conditions for a nonempty subset of a vector space to be a subspace are independent: the set of all vectors in R3 all entries of which are integers is closed under vector addition but not under scalar   a multiplication; the set of all vectors  b  ∈ R3 satisfying abc = 0 is c closed under scalar multiplication but not under vector addition. Example: Let V be a vector space over a field F and let Ω be a nonempty set. We have already seen that the set V Ω of all functions from Ω to V is a vector space over F. If Λ is a subset of Ω then the set {f ∈ V Ω | f (i) = 0V for all i ∈ Λ} is a subspace of V Ω . In particular, if k k < n are positive integers, then   we can think of V as being a subspace       v1       . n n of V , by identifying it with  ..  ∈ V vk+1 = . . . = vn = 0V .         vn Note that if y ∈ V, then {f ∈ V Ω | f (i) = y for all i ∈ Λ} is not a subspace of V Ω unless y = 0V . of vector spaces over a Example: Let {Vi | i ∈ Ω} be a collection field F. The set of all functions f ∈ i∈Ω Vi satisfying the condition that f (i) = 0Vi for at most finitely-many elements i of Ω is a subspace of i∈Ω Vi , called the direct coproduct of the spaces V i and denoted by i∈Ω Vi . The direct coproduct is a proper subset of i∈Ω Vi when and only when the set Ω is infinite. If each of the spaces V i is equal to a given vector space V, we write V (Ω) instead of i∈Ω Vi .


23

Example: If V is a vector space over a field F and if v ∈ V, then the set F v = {av | a ∈ F } is a subspace of V which is contained in any subspace of V containing v. Example: Let R be the field of real numbers and let Ω be either equal to R or to some closed interval [a, b] on the real line. We have already seen that the set RΩ of all functions from Ω to R is a vector space over R. The set of all continuous functions from Ω to R is a subspace of this vector space, as are the set of all differentiable functions from Ω to R, the set of all infinitely-differentiable functions from Ω to R, and the set of all analytic functions from Ω to R. If a < b are real numbers, we will denote the space of all continuous functions from the closed interval [a, b] to R by C(a, b). These spaces will be very important to us later4 . (3.3) Proposition: If V is a vector space over a field F , then a nonempty subset W of V is a subspace of V if and only if it is closed under addition and scalar multiplication. Proof: If W is a subspace of V then it is surely closed under addition and scalar multiplication. Conversely, suppose that it is so closed. Then for any w ∈ W we have 0V = 0w ∈ W and −w = (−1)w ∈ W. All of the other conditions are satisfied in W because they are satisfied in V. (3.4) Proposition: If V is a vector space over a field F , and if {Wi | i ∈ Ω} is a collection of subspaces of V, then i∈Ω Wi is a subspace of V. Proof: Set W = i∈Ω Wi . If w, y ∈ W then, for each i ∈ Ω, we have w, y ∈ Wi and so w + y ∈ Wi . Thus w + y ∈ W. Similarly, if a ∈ R and w ∈ W then aw ∈ Wi for each i ∈ Ω, and so aw ∈ W. We will also set the convention that the intersection of an empty collection of subspaces of V is V itself. Subspaces W and W are disjoint if and only if W ∩ W = {0V }. More generally, a collection {Wi | i ∈ Ω}

4 The first fundamental research in spaces of functions was done by the German mathematician Erhard Schmidt, a student of David Hilbert, whose work forms one of the bases of functional analysis.

24


of subspaces of V is pairwise disjoint if and only if Wi ∩ Wj = {0V } for i = j in Ω. (Note that disjointness of subspaces of a given space is not the same as disjointness of subsets!) Now let us look at a very important method of constructing subspaces of vector spaces. Let D be a nonempty set of elements of a vector space V over a field F. A vector v ∈ V is a linear combination of elements of D over F if and only if there exist elements v1 , . . . , vn of D and n scalars a1 , . . . , an in F such that v = i=1 ai vi . We will denote the set of all linear combinations of elements of D over F by F D. Note that if v ∈ V then F {v} is the set F v which we defined earlier. It is clear that if D is a nonempty set of elements of a vector space V over a field F then D ⊆ F D. Also, 0V ∈ F D for any nonempty subset D of V, and it is the only vector belonging to each of the sets F D. To simplify notation, we will therefore define F ∅ to be {0V }. If D ⊆ D then surely F D ⊆ F D. We also note that F D = F (D ∪ {0V }) for any subset D of V.         3  0   0  1 Example: If D =  0  ,  1  and D =  2  ,  3      0 0 0 0     a  are subsets of R3 , then F D = F D =  b  a, b ∈ R . Indeed,   0   a if  b  ∈ R3 then 0           0 3 a 1 0 a b − a  2  +  3 .  b  = a 0  + b 1  = 2 3 0 0 0 0 0         2 2 1   0 Example: If D =  0  ,  2  ,  0  ,  1  ⊆ R3 then   4 0 0 1         4 0 2 2  2  = 1 0  + 1 2  + 1 0  4 4 0 0       2 2 1 = 1  0  + (−1)  2  + 4  1  . 0 0 1 Thus we see that there may be several ways of representing a vector as a linear combination of elements of a given subset of a vector space.


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(3.5) Proposition: Let D be a subset of a vector space V over a field F. Then: (1) F D is a subspace of V ; (2) Every subspace of V containing D also contains F D; (3) F D is the intersection of all subspaces of V containing D. Proof: If D = ∅ then F D = {0V } and we are done. Thus we can assume that D is nonempty. It is an immediate consequence of the definitions that the sum of two linear combinations of elements of D over F is again a linear combination of elements of D over F, and that the product of a scalar and a linear combination of elements of D over F is again a linear combination of elements of D over F. This proves (1). Moreover, (2) is an immediate consequence of (1) and Proposition 3.3, while (3) follows directly from (2). If D is a subset of a vector space V over a field F then the subspace F D of V is called the subspace generated or spanned by D, and the set D is called a generating set or spanning set for this subspace. In particular, we note that ∅ is a generating set for {0V }.       0 0   1  0 , 1 , 0  Example: Let F be a field. The set is a   0 0 1 generating set for the vector space F 3 over F. The set       1 0   1  1 , 0 , 1    0 1 1 is also a generating set for F 3 if the characteristic of F is other than 2,   1 but not for F = GF (2) since, in this case,  0  cannot be written as 0 a linear combination of this set of vectors over F. The set       0 1   1  0 , 1 , 1    0 0 0 

 0 is not a generating set for F 3 , for any field F, since  0  cannot be 1 written as a linear combination of the elements of this set.

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(3.6) Proposition: Let V be a vector space over a field F and let D1 and D2 be subsets of V satisfying D1 ⊆ D2 ⊆ F D1 . Then F D1 = F D2 . Proof: Since F D1 is a subspace of V containing D2 , we know by Proposition 3.5 that F D2 ⊆ F D1 . Conversely, any linear combination of elements of D1 over F is also a linear combination of elements of D2 over F and so F D1 ⊆ F D2 , thus establishing equality. In particular, we note that F D = F (F D) for any subset D of V. (3.7) Proposition (Exchange Property): Let V be a vector space over a field F and let v, w ∈ V. Let D be a subset of V satisfying v ∈ F (D ∪ {w}) F D. Then w ∈ F (D ∪ {v}). Proof: Since v ∈ F (D ∪ {w}) we know that there exist elements v1 , . . . , vn of D and scalars a1 , . . . , an , b in F satisfying the condition n Moreover, since v ∈ / F D, we know that b = 0 that v = i=1 ai vi + bw. n and so w = b−1 v − i=1 b−1 ai vi ∈ F (D ∪ {v}). A vector space V over a field F is finitely generated over F if it has a finite generating set. Finitely-generated vector spaces are often much easier to deal with by purely algebraic methods and therefore, in several situations, we will have to restrict our discussion to these spaces. Example: If       1          0    0   that   ,    ..      .        0

F is a field and n is a positive integer, then one sees    0 0     0   1       0  0  is a finite generating set for F n over  ,...,   ..   ..    .  .     0 1  

F, and so F n is finitely generated. More generally, if V is a vector space finitely generated over a field F, say V = F {v1 , . . . , vk }, and if n is a positive integer, then             0 0 v2 vk 0 v1     vk   0   v1   v2   0   0               ..  ,  ..  , . . . ,  ..  ,  ..  ,  ..  , . . . ,  ..  , . . .   .   .   .   .   .   .     0 0 0 0 0 0         0 0 0     0   0   0         ..  ,  ..  , . . . ,  ..   .   .   .     v2 vk  v1 


27

is a generating set for V n having kn elements. Example: If F is a field and if k and n are positive integers, then the vector space Mk×n (F ) of all k × n matrices over F is finitely generated over F. Similarly, if V is a finitely-generated vector space over F, then the vector space Mk×n (V ) is also finitely generated over F. Example: For any field F, the vector space F ∞ is not finitely generated over F. Example: The field R is finitely generated as a vector space over itself, but is not finitely generated as a vector space over Q. Let V be a vector space over a field F . In Proposition 3.4, we saw that if {Wi | i ∈ Ω} is a collection of subspaces of V then i∈Ω Wi is a subspace of V. In the same way, we can define the subspace i∈Ω Wi of V to be the set of all vectors in V of the form w , where Λ j j∈Λ ∈ W for each j ∈ Λ. In other is a finite nonempty subset of Ω and w j j words, i∈Ω Wi = F i∈Ω Wi . Indeed, from the definition of this sum, we see something stronger:if Di is a generating set for Wi for each i ∈ Ω then i∈Ω Wi = F i∈Ω Di . As a special case of the above, we see that if W1 and W2 are subspaces of V, then W1 + W2 equals the set of all vectors of the form w1 + w2 , where w1 ∈ W1 and w2 ∈ W2 . If both W1 and W2 are finitely generated then W1 + W2 is also finitely generated. By induction, we can then show that if W1 , . . . , Wn are finitely-generated subspaces of V, then n i=1 Wi is also finitely generated. (3.8) Proposition: If V is a vector space over a field F and if {Wi | i ∈ Ω} is a collectionof of subspaces of V, then: (1) Wh is a subspace of i∈Ω Wi for all h ∈ Ω; (2) If Y is a subspace of V satisfying the condition that Wh is a subspace of Y for all h ∈ Ω, then i∈Ω Wi is a subspace of Y. Proof: (1) is clear from the definition. As for (2), if we have a subspace Y satisfying the given condition, if Λ is a finite subset of Ω, and if wj ∈ W j for each j ∈ Λ, then wj ∈ Y for each j and so j∈Λ wj ∈ Y. Thus i∈Ω Wi ⊆ Y. (3.9) Proposition: If V is a vector space over a field F and if W1 , W2 , and W3 are subspaces of V, then: (1) (W1 + W2 ) + W3 = W1 + (W2 + W3 ); (2) W1 + W2 = W2 + W1 ; (3) W3 ∩ [W2 + (W1 ∩ W3 )] = (W1 ∩ W3 ) + (W2 ∩ W3 );

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(4) (Modular law for subspaces): If W1 ⊆ W3 then W3 ∩ (W2 + W1 ) = W1 + (W2 ∩ W3 ).

Proof: Parts (1) and (2) follow immediately from the definition, while (4) is a special case of (3). We are therefore left to prove (3). Indeed, if v belongs to W3 ∩ [W2 + (W1 ∩ W3 )] , then we can write v = w2 + y, where w2 ∈ W2 and y ∈ W1 ∩ W3 . Since v, y ∈ W3 , it follows that w2 = v − y ∈ W3 , and so v = y + w2 ∈ (W1 ∩ W3 ) + (W2 ∩ W3 ). Thus we see that W3 ∩ [W2 + (W1 ∩ W3 )] ⊆ (W1 ∩ W3 ) + (W2 ∩ W3 ). Conversely, assume that v ∈ (W1 ∩ W3 ) + (W2 ∩ W3 ). Then, in particular, v ∈ W3 and we can write v = w1 + w2 , where w1 ∈ W1 ∩ W3 and w2 ∈ W2 ∩ W3 . Thus v = w1 + w2 ∈ W3 ∩ W2 + (W1 ∩ W3 ). This shows that (W1 ∩ W3 ) + (W2 ∩ W3 ) ⊆ W3 ∩ [W2 + (W1 ∩ W3 )] and so we have the desired equality.

Exercises √ Exercise 48 Let V = Q2 , with the usual vector addition. If a + b 2 ∈ ! ! ! √ √ c c ac + 2bd 2 Q( 2) and if ∈ Q , set a + b 2 = . Do d d bc + ad √ these operations turn Q2 into a vector space over Q( 2)? Exercise 49 Is it possible to define on V = Z/(4) the structure of a vector space over GF (2) in such a way that the vector addition is the usual addition in Z/(4)? Exercise 50 Consider the set Z of integers, together with the usual addition. If a ∈ Q and k ∈ Z, define a · k to be a k, where a denotes the largest integer less than or equal to a. Using this as our definition of “scalar multiplication”, have we turned Z into a vector space over Q? Exercise 51 Let V = {0, 1} and let F = GF (2). Define vector addition and scalar multiplication by setting v + v = max{v, v }, 0v = 0, and 1v = v for all v, v ∈ V. Does this define on V the structure of a vector space over F ? Exercise 52 Let V = C(0, 1). Define an operation on V by setting f g : x → max{f (x), g(x)}. Does this operation of vector addition, together with the usual operation of scalar multiplication, define on V the structure of a vector space over R?


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Exercise 53 Let V = {0V } be a vector space over R. For each v ∈ V and each complex number a + bi, let us define (a + bi)v = av. Does V, together with this new scalar multiplication, form a vector space over C? Exercise 54 Let V = {i ∈ Z | 0 ≤ i < 2n } for some given positive integer n. Define operations of vector addition and scalar multiplication on V in such a way as to turn it into a vector space over the field GF (2). Exercise 55 Let V be a vector space over a field F. Define a function from GF (3) × V to V by setting (0, v) → 0V , (1, v) → v, and (2, v) → −v for all v ∈ V. Does this function, together with the vector addition in V, define on V the structure of a vector space over GF (3)? Exercise 56 Let V = R ∪ {∞} and extend the usual addition of real numbers by defining v + ∞ = ∞ + v = ∞ for all v ∈ V. Is it possible to define an operation of scalar multiplication on V in such a manner as to turn it into a vector space over R? ! ! a a 2 ∈ V and r ∈ R, set , Exercise 57 Let V = R . If b b ! ! ! ! ! a a a + a + 1 a ra + r − 1 + = and r = . Do b b rb b b + b these operations define on V the structure of a vector space over R? If so, what is the identity element for vector addition in this space? Exercise 58 Let V = R and let ◦ be an operation on R defined by a ◦ b = a3 b. Is V, together with the usual addition and “scalar multiplication” given by ◦, a vector space over R? Exercise 59 Show that Z cannot be turned into a vector space over any field. Exercise 60 Let V be a vector space over the field GF (2). Show that v = −v for all v ∈ V. Exercise 61 Give an example of a vector space having exactly 125 elements. Exercise 62 In the definition of a vector space, show that the commutativity of vector addition is a consequence of the other conditions. Exercise 63 Let W be the subset of R5 consisting of all vectors an odd number of the entries in which are equal to 0. Is W a subspace of R5 ? Exercise 64 Let V = RR and let W be the subset of V containing the constant function x → 0 and all of those functions f ∈ V satisfying the condition that f (a) = 0 for at most finitely-many real numbers a. Is W a subspace of V ?

30


    Exercise 65 Let V =   

    a1 a1   ..  0 < a ∈ R . If v =  ..  and  .  i .    a5 a5     b1 a 1 b1     w =  ...  belong to V, and if c ∈ R, set v + w =  ...  and b5 a5 b5  c  a1  ..  cv =  .  . Do these operations turn V into a vector space over R? ac5 Exercise 66 Let F = GF (3).       space of F 3 generated by   

How many elements are there in the sub     1 2  2 , 2  ?  1 1  

Exercise 67 A function f ∈ RR is piecewise constant if and only if it is a constant function x → c or there exist a1 < a2 < . . . < an and c0 , . . . , cn in R such that   c0 if x < a1 ci if ai ≤ x < ai+1 for 1 ≤ i < n . f : x →  cn if an ≤ x Does the set of all piecewise constant functions form a subspace of the vector space RR over R? Exercise 68 Let V be the vector space of all continuous functions from R to itself and let W be the subset of all those functions f ∈ V satisfying the condition that |f (x)| ≤ 1 for all −1 ≤ x ≤ 1. Is W a subspace of V? Exercise 69 Let F = GF (2) and let W be the subspace of F 5 con  a1 5   sisting of all vectors  ...  satisfying i=1 ai = 0. Is W a subspace a5 of F 5 ? Exercise 70 Let V = RR and let W be the subset of V consisting of all monotonically-increasing or monotonically-decreasing functions. Is W a subspace of V ? Exercise 71 Let V = RR and let W be the subset of V consisting of the constant function a → 0, and all epic functions. Is W a subspace of V ?


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Exercise 72 Let V = RR and let W be the subset of V containing the constant function a → 0 and all of those functions f ∈ V satisfying the condition that f (π) > f (−π). Is W a subspace of V ? Exercise 73 Let V = RR and let W be the subset of V consisting of all functions f satisfying the condition that there exists a real number c (which depends on f ) such that |f (a)| ≤ c|a| for all a ∈ R. Is W a subspace of V ? Exercise 74 Let V = RR and let W be the subset of V consisting of all functions f satisfying the condition that there exist real numbers a and b such that |f (x)| ≤ a| sin(x)| + b| cos(x)| for all x ≥ 0. Is W a subspace of V ? Exercise 75 Let F be a field and let V = F F , which is a vector space over F. Let W be the set of all functions f ∈ V satisfying f (1) = f (−1). Is W a subspace of V ? Exercise 76 For any real number 0 < t ≤ 1, let Vt be the set of all functions f ∈ RR satisfying the condition that if a < b in R then there t exists a real number u(a, b) satisfying |f (x) − f (y)| ≤ u(a, b) |x − y| for all a ≤ x, y ≤ b. For which values of t is Vt a subspace of RR ? Exercise 77 Let U be a nonempty subset of a vector space V. Show that U is a subspace of V if and only if au + u ∈ U for all u, u ∈ U and a ∈ F. Exercise 78 Let V be a vector space over a field F and let v and w be distinct vectors in V. Set U = {(1 − t)v + tw | t ∈ F }. Show that there exists a vector y ∈ V such that {u + y | u ∈ U } is a subspace of V. Exercise 79 Let V be a vector space over a field F and let W and Y ! v ∈ V 2 satisfying be subspaces of V 2 . Let U be the set of all vectors v ! v ∈W the condition that there exists a vector v ∈ V such that v ! v ∈ Y. Is U a subspace of V 2 ? and v Exercise 80 Consider R as a vector space over Q. Given a nonempty subset W of R, let W be the set of all real numbers b for which there exists a sequence a1 , a2 , . . . of elements of W satisfying lim ai = b. Show that W is a subspace of R whenever W is.

i→∞

Exercise 81 Let V be a vector space over a field F and let P be the collection of all subsets of V, which we know is a vector space over GF (2). Is the collection of all subspaces of V a subspace of P ?

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Exercise 82 Let W be the set of all functions f ∈ RN satisfying the condition that if f (i) = 0 then f (ji) = 0 for all positive integers j. Is W a subspace of RN ? Exercise 83 Let W be the set of all functions f ∈ RN satisfying the condition that if f (i) = 0 then f (ji) = 0 for all positive integers j. Is W a subspace of RN ? Exercise 84 Let V be a vector space over a field F and let Y be the   v1 v2 0V set of all matrices of the form  0V v1 + v2 0V  in M3×3 (V ). Is 0V v1 v2 Y a subspace of M3×3 (V )? Exercise 85 Let W be the set of all functions f ∈ RR satisfying the following conditions: there exist positive real numbers a and b such that for all x ∈ R satisfying |x| ≥ a we have |f (x)| ≤ b|x|. Show that W is a subspace of RR . Exercise 86 Let W be a subspace of a vector space V over a field F. Is the set (V W ) ∪ {0V } necessarily a subspace of V ? Exercise 87 Let V be a vector space over a field F and let f be a function from V to the unit interval [0, 1] on the real line satisfying the condition that f (au + bv) ≥ min{f (u), f (v)} for all a, b ∈ F and all u, v ∈ V. Show that f (0V ) ≥ f (v) for all v ∈ V and that if 0 ≤ h ≤ f (0V ) then Vh = {v ∈ V | f (v) ≥ h} is a subspace of V. Exercise 88 Find subsets D and D of R3 such that R(D ∩ D ) = RD ∩ RD . Exercise 89 Find subspaces W and Y of R3 having the property that W ∪ Y is not a subspace of R3 . Exercise 90 Let V be a vector space over a field F and let 0V = w ∈ V. Given a vector v ∈ V F w, find the set G of all scalars a ∈ F satisfying F {v, w} = F {v, aw}. Exercise 91 Let p be a prime integer and let V be a vector space over F = GF (p). Show that V is not the union of k subspaces, for any k ≤ p. Exercise 92 Let V be a vector space over a field F and let c and d be fixed elements of F. Define a new operation on V by setting v v = cv + dv . Is V , with this new vector addition and the old scalar multiplication, still a vector space over F ?

4 Algebras over a field

In general, a vector space does not carry with it the notion of multiplying two vectors in the space to produce a third vector. However, sometimes such multiplication may be possible. A vector space K over a field F is an F -algebra if and only if there exists a function (v, w) → v • w from K × K to K such that (1) u • (v + w) = u • v + u • w; (2) (u + v) • w = u • w + v • w; (3) a(v • w) = (av) • w = v • (aw) for all u, v, w ∈ K and a ∈ F. As in the proof of Proposition 2.3(1), these conditions suffice to show that 0K • v = v • 0K = 0K for all v ∈ K. Note that the operation • need not be associative, nor need there exist an identity element for this operation. When the operation is associative, i.e. when it satisfies (4) v • (w • y) = (v • w) • y for all v, w, y ∈ K, then the algebra is called an associative F -algebra. If an identity element for • exists, that is to say, if there exists an element 0K = e ∈ K satisfying v • e = v = e • v for all v ∈ K, we say the F -algebra K is unital. In a unital F -algebra, as with the case of fields, the identity element must be unique. In this case, we can then identify F with the subset {ae | a ∈ F } of K and we note that a • v = v • a for all v ∈ K and a ∈ F. If v is an element of an associative F -algebra (K, •) and if n is a positive integer, we write v n instead of v • . . . • v (n factors). If K 33

34

4. Algebras over a field

is also unital and has a multiplicative identity e, we set v 0 = e for all 0K = v ∈ K. The element (0K )0 is not defined. If v • w = w • v for all v and w in some F -algebra K, then the algebra is commutative. An F -algebra (K, •) satisfying the condition that v • w = −w • v for all v, w ∈ K is anticommutative. If the characteristic of F is other than 2, it is easy to see that this condition is equivalent to the condition that v • v = 0K for all v ∈ K. Of course, in that case K cannot possibly be unital.1 If (K, •) is an associative unital F -algebra having a multiplicative identity e, and if v ∈ K satisfies the condition that there exists an element w ∈ K such that v • w = w • v = e, then we say that v is a unit of K. As with the case of fields, such an element w, if it exists, is unique and is usually denoted by v −1 . If v is a unit, then so is −v, for one −1 immediately notes that (−v) = −(v −1 ). Also, it is easy to see that if v and w are units of K, then so is v • w. Indeed, (v • w) • (w−1 • v −1 ) = (v • (w • w−1 )) • v −1 = (v • e) • v −1 = v • v −1 = e and similarly (w−1 • v −1 ) • (v • w) = e, and so (v • w)−1 = w−1 • v −1 . If v ∈ K is a unit and if n > 1 is an integer, we write v −n instead of (v −1 )n . Example: Any vector space V over a field F can be turned into an associative and commutative F -algebra which is not unital by setting v • w = 0V for all v, w ∈ V. Example: If F is a subfield of a field K, then K has the structure of an associative F -algebra, with multiplication being the multiplication √ in K. Thus, C is an R-algebra and Q( p) is a Q-algebra for every prime integer p. These algebras are, of course, unital.

1

The first systematic study of associative algebras was initiated by the 19th century American mathematician Benjamin Peirce and continued by his son, the mathematician and logician Charles Sanders Peirce. Other major contributors at the beginning of the 20th century were the American mathematician Leonard Dickson and the Scottish mathematician Joseph Henry Wedderburn.


35

Example: Let F be a field, let (K, •) be an F -algebra, and let Ω be a nonempty set. Then the vector space K Ω of all functions from Ω to K has the structure of an F -algebra with respect to the operation • defined by f • g : i → f (i) • g(i) for all i ∈ Ω. This F -algebra is associative if K is. If K is unital with multiplicative identity element e, then K Ω is also unital, with identity element given by the constant function i → e. In particular, if F is a field and if Ω is a nonempty set then F Ω is an associative unital F -algebra with respect to the operation • defined by f • g : i → f (i)g(i) for all i ∈ Ω. Example: We have already seen that the collection of all subsets of a given nonempty set A is a vector space over GF (2). It is in fact an associate and commutative unital GF (2)-algebra with respect to the operation ∩. The identity element with respect to this operation is A itself. Example: Let K be the vector space over R consisting of all functions in RR which are infinitely differentiable, and define an operation • on K by setting f • g = (f g) (where denotes differentiation). Then (K, •) is an algebra which is commutative but not associative. The collection of all operations • on a vector space V over a field F which turn V into an F -algebra will be studied in more detail in Chapter 20. Let F be a field. If (K, •) is an F -algebra, then a subspace L of K satisfying the condition that w • w ∈ L for all w, w ∈ L is an F -subalgebra of K. If (K, •) is a unital F -algebra, then L is a unital subalgebra if it contains the multiplicative identity element of K. Let F be a field. An anticommutative F -algebra (K, •) is a Lie algebra2 over F if and only if it satisfies the additional condition

2 Sophus Lie was a 19th-century Norwegan mathematician who developed mathematical concepts that provide the basic model for quantum theory and an important tool in differential geometry. Another pioneer in the study of noncommutative algebras because of their importance in physics was 20th-century British mathematician Dudley Littlewood.

36


(Jacobi identity) u • (v • w) + v • (w • u) + w • (u • v) = 0K ; for all u, v, w ∈ K. This algebra is not associative unless u • v = 0K for all u, v ∈ K. Example: Let F be a field and let (K, ∗) be an associative F -algebra. Define a new operation • on K by setting v • w = v ∗ w − w ∗ v. Then (K, •) is a Lie algebra over F, which is usually denoted by K − . The operation in K − is known as the Lie product defined on the given F algebra K. This example is very important, because one can show that any Lie algebra over a field F can be considered as a subalgebra of a Lie algebra of the form K − for some associative F -algebra K. (A proof of this result, known as the Poincar´ e-Birkhoff-Witt Theorem, is far beyond the scope of this book.) If v, w ∈ K, then v • w = 0K precisely when v ∗ w = w ∗ v, in other words, precisely when (v, w) forms a commuting pair. Of course, if the algebra K is commutative, all pairs of elements commute, but in general that will not be the case. Lie algebras are of fundamental importance in the modeling problems in physics, and have many other applications; they are in the forefront of current mathematical research. One particular Lie algebra defined on R3 goes back to the work of Grassmann. Define the structure of an R-algebra on R3 with multiplication × given by       a1 b1 a2 b3 − a3 b2  a2  ×  b2  =  a3 b1 − a1 b3  . a3 b3 a1 b2 − a2 b1 This operation, called the cross product, has very important applications in physics and engineering. It is easy to check that the algebra (R3 , ×) is a Lie algebra over R.       1 0 0 Note that if v1 =  0  , v2 =  1  , and v3 =  0  , then, surely, 0 0 1 v1 × v2 = v3 , v1 × v2 = v3 , and v3 × v1 = v2 . Moreover, the cross product is the only possible anticommutative product which can be defined on R3 and which satisfies this condition. Indeed, if • is any such product defined on R3 then      # 3 " 3 3 3 a1 b1  a2  •  b2  = ai vi  bj vj  = ai bj (vi • vj ) i=1 j=1 i=1 j=1 a3 b3       a2 b3 − a3 b2 a1 b1 =  a3 b1 − a1 b3  =  a2  ×  b2  . a1 b2 − a2 b1 a3 b3


37

(4.1) Proposition: If v and w are nonzero elements of R3 ,   0 then v × w =  0  if and only if Rv = Rw. 0    b1 a1 Proof: Suppose v =  a2  and w =  b2 . These vectors are a3 b3 

nonzero and so one of the entries in w is nonzero; without loss of generality, we can assume that b1 = 0. Then a2 b3 −a3 b2 = a3 b1 −a1 b3 = a1 b2 −a2 b1 = 0 and so, if we define c = a1 b−1 1 , we have v = cw. Hence v ∈ Rw. Moreover, c = 0 so w = c−1 v ∈ Rv, proving the desired equality. Conversely, if Rv = Rw then there exists an 0 = d ∈ R such that   0 w = dv. Then v × w = d(v × v) =  0  . 0 The cross product is very particular to the vector space R3 , and does not generalize easily to spaces of the form Rn for n > 3, with the exception of n = 7, which we will see in a later chapter. An important non-associative algebra is the following: let F be a field of characteristic other than 2, and let (K, ∗) be an associative algebra. We can define a new operation • on K, called the Jordan product, by setting v • w = 12 (v ∗ w + w ∗ v). Then (K, •) is a commutative F -algebra, usually denote by K + , called the Jordan algebra defined by K. It is not associative in general, but does satisfy the (Jordan identity)

(v • w) • (v • v) = v • (w • (v • v))

for all v, w ∈ K. Jordan algebras have important applications in physics3 . Note that if v ∗ w = w ∗ v, then v • w = v ∗ w. This observation will have important consequences later.

3 Jordan algebras were developed by 20th-century German physicist Pascual Jordan, one of the fathers of quantum mechanics and quantum electrodynamics. The algebraic structure of Lie algebras and Jordan algebras was studied in detail by 20th-century American mathematicians Nathan Jacobson and A. Adrian Albert.

38


We now come to an extremely important algebra. Let F be a field and let X be an element not in F , which we will call an indeterminate. A polynomial in X with coefficients in F is a formal sum f (X) = ∞ i i=0 ai X , in which the elements ai belong to F , and no more than a finite number of these elements differ from 0. The elements ai are called the coefficients of the polynomial. If all of the ai equal 0, then the polynomial is called the 0-polynomial. Otherwise, there exists a nonnegative integer n satisfying the condition that an = 0 and ai = 0 for all i > n. The coefficient an is called the leading coefficient of the polynomial; the integer n is called the degree of the polynomial, and is denoted by deg(f ). If the leading coefficient of a polynomial is 1, the polynomial is monic. The degree of the 0-polynomial is defined to be −∞, where we assume that −∞ < i for each integer i and (−∞) + i = −∞ for all integers ni. If fi (X) is a polynomial of degree n = −∞, we often write it as i=0 ai X . The set of all polynomials in X with coefficients in F is denoted by F [X]. We identify the elements of F with the polynomials of degree at most 0, and so can consider F as a subdomain of F [X]. We can associate the 0-polynomial with the identity element 0 of F for addition and the polynomials of degree 0 with the nonzero elements of F and so, without any problems, consider F as a subset of F [X]. Example: The polynomials 5X 3 + 2X 2 + 1 and 5X 3 − X 2 + X + 4 in Q[X] both have degree 3 and leading coefficient 5. Therefore they are not monic. The polynomials X 3 + 2X 2 + 1 and X 3 − X 2 + X + 4 in Q[X] are both monic and have the same degree 3. We define addition and multiplication of polynomials over a field as fol∞ ∞ i are polynomials lows: if f (X) = i=0 ai X i and g(X) = i=0 bi X ∞ i , where in F [X], then f (X) + g(X) is the polynomial i=0 ci X ∞ i ci = ai + bi for all i ≥ 0 and f (X)g(X) is the polynomial i=0 di X , i where di = j=0 aj bi−j for all i ≥ 0. It is easy to verify that these definitions turn F [X] into an associative and commutative unital F -algebra with the 0-polynomial acting as the identity element for addition and the degree-0 polynomial 1 acting as the identity element for multiplication. This algebra also has another important property, namely that the product of two nonzero elements of F [X] is again nonzero. An algebra having this property is said to be entire. ∞ ∞ are polynomials in F [X] If f (X) = i=0 ai X i and g(X) = i=0 bi X i ∞ i then we define the polynomial f (g(X)) to be i=0 ai g(X) . Then, for any fixed g(X), the set F [g(X)] = {f (g(X)) | f (X) ∈ F [X]} is a unital subalgebra of F [X]. Commutative, associative, entire, unital F -algebras are integral domains. The converse of this is not true: Z is an integral domain which is not an F -algebra for any field F.


39

Note that every polynomial in F [X] is a linear combination of elements of the set B = {1, X, X 2 , . . .} over F, so B is a set of generators of F [X] over F. On the other hand, it is clear that no finite set of polynomials can be a generating set for F [X] over F, and so F [X] is not finitely generated as a vector space over F. We should remark that the formal definition of multiplication of polynomials does not translate into the fastest method of carrying out such multiplication in practice on a computer, especially for polynomials of large degree. The problem of fast polynomial multiplication has been the subject of extensive research over the years, and many interesting algorithms to perform such multiplication have been devised. A typical such algorithm is Karatsuba’s algorithm4 , which is easy to implement on a computer: let f (X) and g(X) be polynomials in n We can nF [X], where F is a field. write these polynomials as f (X) = i=0 ai X i and g(X) = i=0 bi X i , where n is a nonnegative power of 2 satisfying n ≥ max{deg(f ), deg(g)}. (Of course, in this case an and bn may equal 0.) We now calculate f (X)g(X) as follows: (1) If n = 1 then f (X)g(X) = a1 b1 X 2 + (a0 b1 + a1 b0 )X + a0 b0 . (2) Otherwise, write f (X) = f1 (X)X n/2 + f0 (X) and g(X) = g1 (X)X n/2 + g0 (X), where the polynomials f0 (X), f1 (X), g0 (X), and g1 (X) are all of degree at most n/2. (3) Recursively, calculate f0 (X)g0 (X), f1 (X)g1 (X), and (f0 + f1 )(X)(g0 + g1 )(X). (4) Then f (X)g(X)

4

=

X n (f1 g1 )(X) + X n/2 [(f0 + f1 )(g0 + g1 ) − f0 g0 − f1 g1 ] (X) + (f0 g0 )(X).

Anatoli Karatsuba is a contemporary Russian mathematician whose research is primarily in number theory.

40


Indeed, if the multiplication of two polynomials of degree at most n using the definition of polynomial multiplication takes an order of 2n2 arithmetic operations (i.e., additions and multiplications), it is possible to prove that there exists a fixed positive integer c such that the multiplication of two polynomials of degree at most n using Karatsuba’s algorithm takes at most cn1.59 arithmetic operations. If n is sufficiently large, the difference between these two bounds can be significant. There are other highly-sophisticated algorithms for multiplying two polynomials of degree at most n in an order of n log(n) arithmetic operations. (4.2) Proposition (Division Algorithm): If F is a field and if f (X) and g(X) = 0 are elements of F [X], then there exist unique polynomials u(X) and v(X) in F [X] satisfying f (X) = g(X)u(X) + v(X) and deg(v) < deg(g). ∞ ∞ Proof: Assume that f (X) = i=0 ai X i and g(X) = i=0 bi X i are the given polynomials. If f (X) = 0 or if deg(f ) < deg(g), choose u(X) = 0 and v(X) = f (X), and we are done. Thus we can assume that n = deg(f ) ≥ deg(g) = k, and will prove our result by induction on n. If n = 0 then k = 0 and therefore we can choose u(X) to be a0 b−1 0 , which is a polynomial of degree 0, and choose v(X) to be the 0-polynomial. Now assume, inductively, that n > 0 and that the proposition has been established for all functions f (X) of degree less than n. Set h(X) = n−k g(X). If this is the 0-polynomial, choose u(X) = f (X) − an b−1 k X n−k X and let v(X) be the 0-polynomial. Otherwise, since deg(f ) > an b−1 k deg(h), we see by the induction hypothesis that there exist polynomials v(X) and w(X) in F [X] satisfying h(X) = g(X)w(X) ) + v(X), where ( n−k X + w(X) g(X) + v(X), as deg(g) > deg(v). Thus f (X) = an b−1 k required. We are left to show uniqueness. Indeed, assume that f (X) = g(X)u1 (X) + v1 (X) = g(X)u2 (X) + v2 (X), where deg(v1 ) < deg(g) and deg(v2 ) < deg(g). Then g(X) [u1 (X) − u2 (X)] + [v1 (X) − v2 (X)] equals the 0-polynomial. If u1 (X) = u2 (X) then v1 (X) = v2 (X) and we are done. Therefore assume that u1 (X) = u2 (X). But then, since deg(g[u1 − u1 ]) > deg(v1 − v2 ) and since F [X] is entire, this is a contradiction. Thus we have established uniqueness. Let us emphasize that the set F [X] is composed ∞ of formal expressions and not functions. Every polynomial f (X) = i=0 ai X i ∈ F [X] defines a corresponding polynomial function in F F given by c → f (c) =


41

∞

ai ci , but the correspondence between polynomials and polynomial functions is not bijective. Indeed, it is possible for two distinct polynomials to define the same polynomial function. Thus, for example, if F = GF (2) then the distinct polynomials X, X 2 , X 3 , . . . all define the same function from F to itself, namely the function given by 0 → 0 and 1 → 1. The degree of a polynomial function is the least of the degrees of the (perhaps many) polynomials which define that function.5 i=0

Let p1 (X) and p2 (X) be polynomials in F [X] and let c ∈ F. If we set f (X) = p1 (X) + p2 (X) and g(X) = p1 (X)p2 (X) then it is clear that f (c) = p1 (c) + p2 (c) and g(c) = p1 (c)p2 (c). (4.3) Proposition: Let F be a field and let p(X) be a polynomial in F [X]. Then an element c of F satisfies the condition that p(c) = 0 if and only if there exists a polynomial u(X) ∈ F [X] satisfying p(X) = (X − c)u(X).

Proof: By Proposition 4.2, we know that there exist polynomials u(X) and v(X) in F [X] satisfying p(X) = (X − c)u(X) + v(X), where deg(v) < deg(X − c) = 1. Therefore v(X) = b for some b ∈ F. If b = 0 then p(c) = (c − c)u(c) = 0. Conversely, if p(c) = 0 then 0 = p(c) = (c − c)u(c) + b = b and so p(X) = (x − c)u(X). As an immediate consequence of this result, we see that if F is a field and if p(X) ∈ F [X], then the set of all elements c of F satisfying p(c) = 0 is finite and, indeed, cannot exceed the degree of p(X). Let F be a field. A polynomial p(X) ∈ F [X] is reducible if and only if there exist polynomials u(X) and v(X) in F [X], each of degree at least 1, satisfying p(X) = u(X)v(X). Otherwise, the polynomial is irreducible. Many tests for the irreduciblity of polynomials in Q[X] have been devised. One of the earliest and well-known is Eisenstein’s

5 The first person to systematically consider the best methods of calculating f (c) for a polynomial f (X) ∈ F [X] and for c ∈ F, was the twentiethcentury Russian mathematician Alexander Ostrowski.

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n criterion:6 if p(X) = i=0 ai X i ∈ Q[X], where each ai is an integer, and if there exists a prime integer q such that q does not divide an , q divides ai for all 0 ≤ i ≤ n − 1, and q 2 does not divide a0 , then p(X) is irreducible. (A proof of this can be found in books on abstract algebra.) Thus, using this criterion, we see that 3X 3 + 7X 2 + 49X − 7 is an irreducible polynomial in Q[X]. Example: If F = GF (5) then the polynomial X 3 + X + 1 ∈ F [X] is irreducible, a fact which can be established, if necessary, by testing all possibilities. However, when F = GF (3) it is easy to verify the factorization X 3 + X + 1 = (X + 2)(X 2 + X + 2), and thus see that the polynomial is reducible. Example: If p(X) = u(X)v(X) in F [X], then surely p(X + c) = u(X + c)v(X + c) for any c ∈ F, and so to prove that a polynomial p(X) is irreducible it suffices to prove that p(X + c) is irreducible for some c ∈ F. For example, let q be a prime integer.The qth cyclotomic q−1 polynomial in Q[X] is defined to be Φq (X) = i=0 X i . We claim that this polynomial is irreducible. To see that this is so, we note that Φq (X + 1) = X

q−1

+

q X i, q−1−i

q−2 i=0

which is irreducible by Eisenstein’s criterion. It is known that the number of monic irreducible polynomials of positive 1 µ(d)pm/d , where the sum degree m in GF (p) equals N (p) = m ranges over all integers d which divide m and the M¨ obius function µ(d) is defined by  if d = 1  1 (−1)k if d is the product of k distinct primes . µ(d) =  0 otherwise This means that the probability of a randomly-selected monic polynomial of degree m in GF [X] being irreducible is N (p)/pm , which is roughly 1 m.

6

losis at the age of 29.

Gauss’ brilliant student, Ferdinand Eisenstein, died of tubercu-


43

Any polynomial in F [X] can be written as a product of irreducible polynomials. How to find such a decomposition, especially in the case of polynomials over a finite field or over Q, is a very difficult and important problem, which attracted such great mathematicians as Newton and which continues to attract many important mathematicians until this day. Indeed, the problem of factoring polynomials over finite fields into irreducible components has become even more important, since it is the basis for many current cryptographic schemes. There are algorithms, such as Berlekamp’s algorithm, which factor a polynomial f (X) ∈ F [X], where F = GF (pn ), in a time polynomial in p, n, and deg(f ). Moreover, under various assumptions, such as the Generalized Riemann Hypothesis, polynomials of special forms can be factored much more rapidly. A polynomial p(X) ∈ F [X] of positive degree is completely reducible if and only if it can be written as a product of polynomials in F [X] of degree 1. Not every polynomial over every field is completely reducible. For example, the polynomial X 2 + 1 ∈ Q[X] is not completely reducible. The field F is algebraically closed if every polynomial of positive degree in F [X] is completely reducible. The fields Q and R are not algebraically closed. The field C is algebraically closed, by a theorem known as the Fundamental Theorem of Algebra. This theorem is in fact analytic and not algebraic, and relies on various analytic properties of functions of a complex variable. Most of the great mathematicians of the eighteenth century – d’Alembert, Euler, Laplace, Lagrange, Argand, Cauchy, and others – tried in vain to prove this theorem. The first proof was given by Gauss in his doctoral thesis in 1799. His proof was basically topological and relied on work of Euler. During his lifetime, Gauss published several proofs of this theorem7 . Example: The field F = GF (2) is not algebraically closed since the polynomial X 2 + X + 1 ∈ F [X] is not completely reducible. Note that if a field F is algebraically closed then every polynomial function F → F defined by a polynomial of positive degree is epic. Indeed, let p(X) ∈ F [X] be a polynomial of positive degree and let d ∈ F. Then

7

Most proofs of the Fundamental Theorem of Algebra are existence proofs and do not give a constructive method of finding the degree-one factors of a polynomial over an algebraically-closed field. The first constructive proof was given by the German mathematician Helmut Kneser in 1940.

44


q(X) = p(X) − d is a polynomial of positive degree in F [X] and so there exists an element c of F such that q(c) = 0. In other words, p(c) = d. (4.4) Proposition: A monic polynomial p(X) ∈ R[X] is irreducible if and only if it is of the form X − a or (X − a)2 + b2 , where a ∈ R and 0 = b ∈ R. Proof: Clearly every polynomial of the form X − a is irreducible. Now assume that f (X) = (X − a)2 + b2 = X 2 − 2aX + a2 + b2 . Were this polynomial reducible, we could find real numbers c and d satisfying f (X) = (X − c)(X − d) = X 2 − (c + d)X + cd and so c+d = 2a* and cd = a2 +b2 . This implies that c2 −2ac+a2 +b2 = 0 + √ 1 2 2 2 and hence c = 2 2a ± 4a − 4(a + b ) = a± −b2 , which contradicts the assumption that c ∈ R since b is assumed to be nonzero. Thus polynomials of both of the given forms are indeed irreducible. n Conversely, let p(X) = i=0 ci X i be a monic irreducible polynomial in R[X] that is not of the form X − a. By the Fundamental Theorem of Algebra we know that there exists a complex number z = a + bi satisfying p(z) = 0. Since the coefficients of p(X) are real, this means that p(z) = 0 n i as well, since 0 = 0 = p(z) = i=0 ci z = p(z). Thus there exists a polynomial u(X) ∈ R[X] satisfying p(X) = (X − z)(X − z)u(X), where (X − z)(X − z) = X 2 − (z + z)X + zz = X 2 − 2aX + a2 + b2 . Since p(X) was assumed irreducible, we conclude that z ∈ / R (i.e. b = 0) and that p(X) equals X 2 − 2aX + a2 + b2 , as desired. An obvious generalization of the above construction is the following: let F be a field and let (K, •) be an F -algebra. If X is an element not in K, we candefine a polynomial with coefficients in K as a formal ∞ sum f (X) = i=0 ai X i , in which the elements ai belong to K and no more than a finite number of them differ from 0K . The set of all such polynomials will be denoted by K[X]. As above, wedefine addition ∞ i and and multiplication in K[X] as follows: if f (X) = i=0 ai X ∞ i b X belong to K[X], then f (X) + g(X) is the polynomial g(X) = i i=0 ∞ i c = ai + bi for each 0 ≤ i ≤ ∞, and f (X)g(X) i=0 ci X , in which i ∞i i is the polynomial i=0 di X , in which di = j=0 aj • bi−j for each 0 ≤ i ≤ ∞. Again, it is easy to check that K[X] is an F -algebra. This generalization allows us to consider algebras of polynomials in several indeterminates with coefficients in K defined inductively by setting K[X1 , . . . , Xn ] = K[X1 , . . . , Xn−1 ][Xn ] for each n > 1. Elements of this algebra are of the form f (X1 , . . . , Xn ) =

ai1 ,...,in X1i1 · . . . · Xnin ,


45

where the sum ranges over all n-tuples (i1 , . . . , in ) of nonnegative integers and at most finitely-many of the coefficients ai1 ,...,in ∈ K are nonzero.

Exercises Exercise 93 Let F be a field and let (K, •) and (L, ∗) be F -algebras. ! ! ! a • a a a = . Is Define an operation on K × L by b b ∗ b b (K × L, ) an F -algebra? Exercise 94 Let F be a field and let (K, •) be a unitary, associative, commutative, and entire F -algebra which, as a vector space, is finitely generated over F. Is K a field? Exercise 95 Let F be a field and let (K, •) be an associative F -algebra which, as a vector space, is finitely generated over F. Given an element a ∈ K, do there necessarily exist elements a1 , a2 ∈ K satisfying a1 • a2 = a? Exercise 96 Define an operation • on R2 by setting ! ! ! a c 2ac − bd • = . b d ad + bc Show that this operation turns R2 into an R-algebra. Is this algebra associative? Exercise 97 Let F be a field and let (K, •) be a unital F -algebra. Define an operation on the vector space L = K × F by setting ! ! ! v w v • w + bv + aw = a b ab for all v, w ∈ K and a, b ∈ F. Is L an F -algebra? Is it unital? Exercise 98 Let F be a field. An F -algebra (K, •) is a division algebra if and only if for every v ∈ K and for every 0K = w ∈ K there exist unique vectors x, y ∈ K, not necessarily equal, satisfying w • x = v and y • w = v. Is the algebra defined in the previous exercise a division algebra? Exercise 99 Let F be a field and let (K, •) be an associative F -algebra which, as a vector space, is finitely generated over F. Suppose that there exists an element y ∈ K satisfying the condition that for each v ∈ K there exists an element v ∈ K satisfying v • y = v. Show that each such element v must be unique.

46


Exercise 100 Let F be an infinite field and let (K, ∗) be an associative unital F -algebra. If v, w ∈ K, show that there are infinitely-many elements w of K satisfying v • w = v • w in K. Exercise 101 Let F be a field and let (K, •) be an associative unital F -algebra. If A and B are subsets of K, we let A • B be the set of all elements of K of the form a • b, with a ∈ A and b ∈ B (in particular, ∅ • B = A • ∅ = ∅). We know that the set V of all subsets of K is a vector space over GF (2). Is (V, •) a GF (2)-algebra? If so, is it associative? Is it unital? Exercise 102 Let F be a field and let (K, •) be an associative F -algebra. If V andW are subspaces, we let V • W be the set of all finite sums of n the form i=1 vi • wi , with vi ∈ V and wi ∈ W. Is V • W necessarily a subspace of K? Exercise 103 For v, w ∈ R3 , simplify the expression (v + w) × (v − w). Exercise 104 For u, v, w ∈ R3 , simplify the expression (u + v + w) × (v + w). Exercise 105 Let F be a field and let (K, •) be an F -algebra satisfying the Jacobi identity. Show that K is a Lie algebra if and only if v •v = 0K for all v ∈ K. Exercise 106 Let F be a field and let (K, ∗) be an associative F algebra. For each 0F = c ∈ F and define an operation •c on K by setting v •c w = c(v ∗ w + w ∗ v). For which values of c is (K, •) a Jordan algebra over F ? Exercise 107 Let F be a field and let (K, •) be a unitary F -algebra. For each v ∈ K, let S(v) be the set of all a ∈ F satisfying the condition that v−a1K does not have an inverse with respect to the operation •. If v ∈ K has a multiplicative inverse v −1 with respect to this operation, show that either S(v) = ∅ = S(v −1 ) or S(v) = ∅ and S(v −1 ) = {a−1 | a ∈ S(v)}. Exercise 108 Let F be a field and let L be the set of all polynomials f (X) ∈ F [X] satisfying the condition that f (−a) = −f (a) for all a ∈ F. Is L a subspace of F [X]? Exercise 109 Let F be a field and let L be the set of all polynomials f (X) ∈ F [X] satisfying the condition that deg(f ) is even. Is L a subspace of F [X]? Exercise 110 Let F be a field and let f (X), g(X) ∈ F [X]. Show that deg(f g) = deg(f ) + deg(g). Exercise 111 Let F be a field and let f (X), g(X) ∈ F [X]. Show that deg(f + g) ≤ max{deg(f ), deg(g)}, and give an example in which we do not have equality.


47

Exercise 112 Find polynomials u(X), v(X) ∈ Q[X] satisfying X 4 + 3X 3 = (X 2 + X + 1)u(X) + v(X). Exercise 113 Let F = GF (2). Find polynomials u(X), v(X) ∈ F [X] satisfying X 5 + X 2 = (X 3 + X + 1)u(X) + v(X). Exercise 114 Let F = GF (7). Find a nonzero polynomial p(X) ∈ F [X] such that the polynomial function defined by p is the 0-function. Exercise 115 Is the polynomial 6X 4 +3X 3 +6X 2 +2X+5 ∈ GF (7)[X] irreducible? Exercise 116 Is the polynomial X 7 + X 4 + 1 ∈ Q[X] irreducible? Exercise 117 Let t ∈ R satisfy the condition that there exist a, b ∈ R satisfying c + d = 1 and 2a3 − a2 − 7a + t = 0 = 2b3 − b2 − 7b + t. Find t. Exercise 118 Compare the subsets F [X 2 ] and F [X 2 + 1] of F [X], where F is a field. Exercise 119 Let F = GF (p), where p is a prime integer, and let g be an arbitrary function from F to itself. Show that there exists a polynomial p(X) ∈ F [X] of degree less than p satisfying the condition that g(c) = p(c) for all c ∈ F. Exercise 120 Let c be a nonzero element of a field F and let n > 1 be an integer. Show that there exists a polynomial p(X) ∈ F [X] satisfying cn + c−n = p(c + c−1 ). Exercise 121 Let F be a field. Find the set of all polynomials 0 = p(X) ∈ F [X] satisfying p(X 2 ) = p(X)2 . Exercise 122 Let k be a positive integer and let pk (X) =

1 X(X − 1) · . . . · (X − k + 1) ∈ Q[X]. k!

Show that pk (n) ∈ Z for every nonnegative integer n. Exercise 123 For any positive integer n, let pn (X) = nX n+1 − (n + 1)X n + 1 ∈ Q[X]. Show that there exists a polynomial qn (X) ∈ Q[X] satisfying pn (X) = (X − 1)2 qn (X).

48


Exercise 124 Let F be a field and let W be a nontrivial subspace of the vector space F [X] over F. Let p(X) ∈ F [X] be a given monic polynomial and let p(X)W = {p(X)f (X) | f (X) ∈ W }. Show that p(X)W is a subspace of F [X] and find a necessary and sufficient condition for it to equal W. Exercise 125 Let p be a prime integer and let n be a positive integer. Does there necessarily exist an irreducible monic polynomial in GF (p)[X] of degree n? Exercise 126 Let p be a prime integer and let n be a positive integer. Show that the product of all irreducible monic polynomials in GF (p)[X] n of degree dividing n is equal to X p − X. Exercise Let n > 1 be an integer. Is the polynomial p(X) = n 127 1 X h ∈ Q[X] necessarily irreducible? 1 + h=1 h! Exercise 128 Show that the polynomial X 4 + 1 is irreducible in Q[X] but reducible in GF (p)[X] for every prime p. Exercise 129 Show that the polynomial in Q[X] of the form X 4 + 2(1 − c)X 2 + (1 + c)2 √ is irreducible for every c ∈ Q satisfying c∈ / Q. Exercise 130 Let k be a positive integer and let a < b be real numbers. A function f ∈ R[a,b] is a spline function of degree k if and only if there exist real numbers a = a0 < . . . < an = b and polynomials p0 (X), . . . , pn−1 (X) of degree k in R[X] satisfying the conditon that f : x → pi (x) for all ai ≤ x ≤ a i+1 and all 0 ≤ i ≤ n − 1. Spline functions play an important part in interpolation theory. Is the set of all spline functions of fixed degree k a subspace of the vector space R[a,b] ?

5 Linear independence and dimension

In this chapter we will see how a restricted group of vectors in a vector space over a field can dictate the structure of the entire space, and we will deduce far-ranging conclusions from this. Let V be a vector space over a field F. A nonempty subset D of V is linearly dependent if and only if there exist distinct vectors v1 , . . . , vn in D and nscalars a1 , . . . , an in F, not all of which are equal to 0, satisfying i=1 ai vi = 0V . A list of elements of V is linearly dependent if it has two equal members or if its underlying subset is linearly dependent. Clearly any set of vectors containing 0V is linearly dependent. A nonempty set of vectors which is not linearly dependent is linearly independent1 . That is to say, D is linearly independent if and only if D = ∅ or D = ∅ and we have n i=1 ai vi = 0V with the ai in F and the vi in V, when and only when ai = 0 for all 1 ≤ i ≤ n. As a consequence of this definition, we

1 The notion of linear independence of vectors was extensively generalized to other mathematical contexts the by 20th-century American mathematician Hassler Whitney.

49

50

5. Linear independence and dimension

see that an infinite set of vectors is linearly dependent if and only if it has a finite linearly-dependent subset, and an infinite set of vectors is linearly independent if and only if each of its finite subsets is linearly independent. It is also clear that any set of vectors containing a linearly-dependent subset is linearly dependent and that any subset of a linearly-independent set of vectors is linearly independent.       −1 −4   1  2 , 3 , 7  Example: The subset of Q3 is lin    1  4  11    0 1 −1 −4 early dependent since  0  = (−1)  2  + 3  3  + (−1)  7  . 0 1 4 11       1 1   1  0 , 1 , 1  Similarly, the subset of Q3 is linearly inde  0 0 1           0 1 1 1 0 pendent, since if  0  = a  0  + b  1  + c  1  , then  0  = 0 0 0 1 0   a+b+c  b + c  and that implies that a = b = c = 0. c              Example: The subset              

1 1 0 1 1 0 0

          ,        

1 0 1 1 0 1 0

          ,        

0 1 1 1 0 0 1

           of GF (2)7 is linearly         

independent and generates a subspace of V composed of eight vectors:          

0 0 0 0 0 0 0

      ,    

        

1 1 0 1 1 0 0

      ,    

        

1 0 1 1 0 1 0

      ,    

        

0 1 1 1 0 0 1

      ,    

        

0 0 0 1 1 1 1

      ,    

        

1 1 0 0 0 1 1

      ,    

        

1 0 1 0 1 0 1





     , and    

        

0 1 1 0 1 1 0

     .    

Note that in every element of V other than its identity element for addition, a majority of the entries are nonzero. This property makes this subspace of V important in algebraic coding theory.


51

Example: Let b˙ > 1 be a real number, let {p1 , p2 , . . .} be the set of prime integers and, for each i, let ui = logb (pi ). We claim that D = {u1 , u2 , . . .} is a linearly-independent subset of R, when it is considered as a vector space over Q. Indeed, assume that this is not the case. Then there is a positive integer n and rational numbers a1 , . . . , an n satisfying i=1 ai ui = 0. If we multiply both sides by the product of the denominators of the ai , we can assume that the ai are integers. Then 1 = b0 = b

ai ui

=

n i=1

bai ui =

n i=1

(bui )

ai

=

n

pai i ,

i=1

and this is a contradiction. Therefore D must be linearly independent. Example: Let F be a field and let Ω be a nonempty set. Let Vi be a vector space over F for each i ∈ Ω, and set V = i∈Ω Vi . We have already seen that the identity for addition in this vector space Ω → i∈Ω Vi given by g0 : i → 0Vi . For each is the function g0 : i ∈ Ω, let fi : Ω → i∈Ω Vi be a function satisfying the condition that fi (i) = g0 (i) but fi (h) = g0 (h) for all h ∈ Ω {i}. We claim that the subset {fi | i ∈ Ω} of V is linearly independent. To see that, assume that there exists a finite subset Λ of Ω and a family of scalars {ch | h ∈ Λ} such that h∈Λ ch fh = g0 . Then for each k ∈ Λ we have g0 (k) = h∈Λ ch fh (k) = h∈Λ ch fh (k) = ck fk (k) and since, by definition, fk (k) = g0 (k), we must have ck = 0. Example: If F is a field, thesubset {1, X, X 2 , . . .} of F [X] is n i surely linearly independent, since i=0 ai X = 0 if and only if each of the coefficients ai equals 0. Example: Let V = RR be the vector space, over R, of all functions from R to itself. Let D be the set of all functions of the form x → eax for some real number a. We claim that D is linearly independent. Indeed, assume that there are distinct real numbers n a1 , . . . , an and real numbers c1 , . . . , cn such that the function x → i=1 ci eai x equals the 0-function f0 : x → 0, which is the identity element of V for addition. We need to show that each of the ci equals 0, and this we will do by induction on n. If n = 1 then we must have c1 = 0 since the function x → eax is different from f0 for each a ∈ R. Assume therefore that n > 1 and that every subset of D having no more than n − 1 elements is linearly independent. For each 1 ≤ i ≤ n, set bi = ai − an . Then n−1 n f0 = e−an x ci eai x = ci ebi x + cn i=1

i=1

52


and if we differentiate both sides of the equation, we see that f0 = n−1 bi x . By the induction hypothesis and the choice of the scalars i=1 bi ci e ai as being distinct, it follows that bi ci = 0 = bi for each 1 ≤ i ≤ n − 1 and so ci = 0 for all 1 ≤ i ≤ n − 1. This in turn implies that cn = 0 as well. Similarly, let G be the subset of V consisting of all of the functions of the form gi : x → xi−1 2x−1 . We claim that this set too is linearly independent. Indeed, assume otherwise. Then there exists a positive integer n , . . . , c , such that n and there exist real numbers c 1 n i=1 ci gi = f0 . n x−1 i−1 = 0 for each real x. c x But this implies that 2 i i=1 n number i−1 Since 2x−1 = 0 for each x ∈ R, we conclude that c x = 0 i i=1 n for all x. But the polynomial function x → i=1 ci xi−1 from R to itself has infinitely-many roots if and only ci = 0 for all i, proving linear independence. Note that if {v, w} is a linearly-dependent set of vectors in an anticommutative algebra (K, •) over a field of characteristic other than 2, then there exist scalars a and b, not both equal to 0, such that av + bw = 0K . Relabeling if necessary, we can assume that b = 0. Then 0K = a(v • v) + b(v • w) = b(v • w) and so v • w = 0K . A simple induction argument shows that if D is a linearly-dependent subset of K then v1 • . . . • vk = 0K for any finite subset {v1 , . . . , vk } of D. Note too that Proposition 3.7 can be easily iterated to get the more general result that if D is a nonempty subset of a vector space V over a field F and if B is a finite linearly-independent subset of F D having k elements, then there exists a subset D of D also having k elements satisfying the condition that F ((D D ) ∪ B) = F D. Moreover, if D is linearly independent, so is (D D ) ∪ B. This result is sometimes known as the Steinitz Replacement Property. (5.1) Proposition: Let V be a vector space over a field F. A nonempty subset D of V is linearly dependent if and only if some element of D is a linear combination of the others over F.

Proof: Assume D is linearly dependent. Then there exists a finite , vn } of D and scalars a1 , . . . , an , not all of which equal subset {v1 , . . . n −1 0, satisfying i=1 ai vi = 0V . Say ah = 0. Then vh = −ah i=h ai vi and so we see that vh is a linear combination of the other elements of D over F. Conversely, assume that there is some element of D is a linear combination of the others over F. That is to say, there is an element v1 of D, elementsv2 , . . . , vn of D {v1 } and scalars a2 , . . . , an in F n n satisfying v1 = i=2 ai vi . If we set a1 = −1, we see that i=1 ai vi = 0V and so D is linearly dependent.


53

Example: For every real number a, let fa be the function in RR defined by fa : x → |x − a|. We claim that the subset D = {fa | a ∈ R} of RR is linearly independent. Indeed, assume that this is not the case. Then there exists a real number b such that fb is a linear combination of other members of D. In other words, there exists a finite subset E of R \ {b} and scalars ca for each a ∈ E such that fb = a∈E ca fa . But the function on the right-hand side of this equation is differentiable at b, while the function on the left-hand side is not. From this contradiction, we see that D is linearly independent. We now introduce a new concept: if A is a nonempty set, then a relation between elements of A is called a partial order relation if and only if the following conditions are satisfied: (1) a a for all a ∈ A; (2) If a b and b a then a = b; (3) If a b and b c then a c. The term “partial” comes from the fact that, given elements a and b of A, it may happen that neither a b nor b a. A set on which a partial order has been defined is a partially-ordered set. A partially-ordered set A satisfying the condition that for all a, b ∈ A we have either a b or b a is called a chain. A nonempty subset B of a partially-ordered set A is itself partially-ordered relative to the partial order relation defined on A; it is a chain subset if it is a chain relative to the partial order defined on A. If A is a nonempty set on which we have a partial order relation defined, then an element a0 of A is maximal in A if and only if a0 a when and only when a = a0 . An element a1 is minimal if and only if a a1 when and only when a = a1 . Maximal and minimal elements need not exist or, if they exist, need not be unique. The Well Ordering Principle, one of the fundamental axioms of number theory, says that any nonempty subset of N, ordered with the usual partial order, has a minimal element. Partial order relations are ubiquitous in mathematics, and often play a very important, though not usually highlighted, part in the analysis of mathematical structures. Example: Let A be a nonempty set and let P be the collection of all subsets of A. Define a relation between elements of P by setting B B if and only if B ⊆ B . It is easy to verify that this is indeed a partial order relation. Moreover, P has a unique maximal element, namely A, and a unique minimal element, namely ∅. The set P is not a chain whenever A has more than one element since, if a and b are distinct elements of A, then {a} {b} and {b} {a}. Example: Let A = {1, 2, 3} and let P be the collection of all subsets of A having one or two elements. Thus P has six elements: {1}, {2},

54


{3}, {1, 2}, {1, 3}, and {2, 3}. Again, the relation between elements of P defined by setting B B if and only if B ⊆ B is a partial order relation. Moreover, P has three minimal elements: {1}, {2}, and {3}; it also has three maximal elements: {1, 2}, {1, 3}, and {2, 3}. In general, if we have a collection of subsets of a given set, the collection is partially-ordered by setting B B if and only if B ⊆ B . Therefore it makes sense for us to talk about “a minimal generating set” of a vector space V – namely a minimal element in the partially-ordered collection of all generating sets of V – and about “a maximal linearly-independent subset” of a vector space V – namely a maximal element of the partiallyordered collection of all linearly-independent subsets of V. However, we have no a priori guarantee that such minimal or maximal elements in fact exist. Example: Consider the set A of all integers greater than 1, and define a relation on A by setting k n if and only if there is a positive integer t satisfying n = tk. This is a partial order relation on A. Moreover, A has infinitely-many minimal elements, since each prime integer is a minimal element of A, while it has no maximal elements, since n 2n for each n ∈ A. (5.2) Proposition: Let V be a vector space over a field F. Then the following conditions on a subset D of V are equivalent: (1) D is a minimal set of generators of V ; (2) D is a maximal linearly-independent subset of V ; (3) D is a linearly-independent set of generators of V . Proof: (1) ⇒ (2): Let D be a minimal set of generators of V, and assume that D is linearly dependent. By Proposition 5.1 there exists an element v0 ∈ D which is a linear n combination of elements of the set E = D {v0 } over F. Say v0 = i=1 ai ui , where the ui belong to E and the ai are scalars in F. If v is arbitrary element of V then, since D is a set of generators of V, there exists elements v1 , . . . , vn of E and n scalars b0 , b1 , . . . , bn such that v = j=0 bj vj . But this then implies that n n n v = b0 v0 + j=1 bj vj = i=1 b0 ai ui + j=1 bj vj and so E is also a set of generators of V, contradicting the minimality of D. This establishes the claim that D is linearly independent. If v ∈ V D, the set D ∪ {v} is linearly dependent since v is a linear combination of elements of D. Thus D is a maximal linearly-independent set. (2) ⇒ (3): Assume that D is a maximal linearly-independent subset of V. Consider a vector v0 in V D. By (2), we know that the set D ∪ {v0 } is linearly dependent and so 0V ∈ F (D ∪ {v0 }) F D by Proposition 3.7, this implies v0 ∈ F (D ∪ {0V }) = F D, which proves that D is a set of generators of V.


55

(3) ⇒ (1): Assume that D is a linearly-independent set of generators of V and that E is a proper subset of D which is also a set of generators for V. Let v0 ∈ D E. Then there exist n elements v1 , . . . , vn of E and scalars a1 , . . . , an such that v0 = i=1 ai vi . But, by Proposition 5.1, that implies that the set D is linearly dependent, contradicting (3). Therefore no such E exists and so D is a minimal set of generators of V. (5.3) Proposition: Let V be a vector space over a field F and let D be a linearly-independent subset of V. If v0 ∈ V F D then the set D ∪ {v0 } is linearly independent. Proof: Assume that this set is linearly dependent. Then there exist . . , vn of D and scalars a0 , a1 , . . . , an , not all equal to elements v1 , . n 0, such that i=0 ai vi = 0V . The scalar a0 must be different from 0, for otherwise D would be linearly dependent, which is a contradiction. n Therefore v0 = i=1 −a−1 0 ai vi ∈ F D, which contradicts the choice of v0 . Thus D ∪ {v0 } must be linearly independent. Proposition 5.3 has important implications. For example, let V be a vector space over a field F which is not finitely generated and let D = {v1 , . . . , vn } be a linearly-independent subset of V. Then F D = V, since V is not finitely generated, and so there exists a vector vn+1 ∈ V F D such that {v1 , . . . , vn+1 } is linearly independent. Thus we see that a vector space which is not finitely generated has linearly-independent finite subspaces of arbitrarily-large size. A generating set for a vector space V over a field F which is also linearly independent, is called a basis of V over F. In Proposition 5.2 we gave some equivalent conditions for determining of a subset of a vector space is a basis. However, we have not yet proven that every (or, indeed, any) vector space must have a basis.       0 0   1  0 , 1 , 0  Example: Clearly and   0 0 1       1 1   1  0 , 1 , 1    0 0 1 are bases of F 3 for any field F.      1  1  1 , 0 , than 2, then  0 1

If the characteristic of F is other  0  1  is a basis of F 3 , but if the  1

56


field F has characteristic 2, then the set is linearly dependent, since         1 1 0 0  1  +  0  +  1  =  0 . 0 1 1 0 Example: Let F be a field and let both k and n be positive integers. For each 1 ≤ s ≤ k and each 1 ≤ t ≤ n, let Hst be the matrix [aij ] in Mk×n (F ) defined by

1 if (i, j) = (s, t) . aij = 0 otherwise Then {Hst | 1 ≤ s ≤ k and 1 ≤ t ≤ n} is a basis of Mk×n (F ). Example: If F is a field, then we have already seen that the subset {1, X, X 2 , . . .} of F [X] is a linearly-independent generating set for F [X] as a vector space over F, and so is a basis of this space. The same is true for the subset {1, X + 1, X 2 + X + 1, . . .} of F [X]. More generally, if {p0 (X), p1 (X), . . .} is a subset of F [X] satisfying the condition that deg(pi (X)) = i for all i ≥ 0, then it is a basis of F [X] as a vector space over F. Since every element of a vector space V over a field F has a unique representation as a linear combination of elements of a basis, if one wants to define a structure of an F -algebra on V it suffices to define the product of any pair of basis elements, and then extend the definition by distributivity and associativity. This is illustrated by the following example, and we will come back to it again in Proposition 5.5. Example: We have already noted that if F is a field then F [X] is an associative F -algebra. Let us generalize this construction. Let H be a nonempty set on which we have defined an associative operation ∗. Thus, for example, H could be the set of nonnegative integers with the operation of addition or multiplication. Let V be the vector space over F with basis {v h | h ∈ H} and define an operation • on V as follows: if v = g∈H ag vg and w = h∈H bh vh are elements of V (where at most of the ag and the bh are nonzero), then finitely-many set v • w = g∈H h∈H ag bh vg∗h . This turns V into an associative F algebra. In the case H = {X i | i ≥ 0}, we get F [X]. Such constructions are very important in advanced applications of linear algebra. Note that a vector space may have (and usually does have) many bases and so the problem arises as to whether there is a preferred basis among all of these. For vector spaces of the form F n , there are reasons to prefer


        the basis         

1 0 0 .. . 0

        ,    

0 1 0 .. . 0





      ,...,    

0 0 0 .. . 1

57

         ; for vector spaces of the form      

Mk×n (F ) there are reasons to prefer the basis {Hst | 1 ≤ s ≤ k and 1 ≤ t ≤ n} defined above; and for vector spaces of the form F [X] there are reasons to prefer the basis {1, X, X 2 , . . .}. These bases are called the canonical bases of their respective spaces. However, in various applications – especially those involving large calculations – it is often convenient and sometimes extremely important to pick other bases which fit the problem under consideration. It is also important to emphasize another point. When we defined the notation for this book, we stressed that when a set is defined by listing its elements, the set comes with an implicit order defined by that listing. When we deal with bases, and especially finite bases, the order in which the elements of the basis are written often plays a critical role, and one should never lose track of this. (5.4) Proposition: Let V be a vector space over a and let D be a nonempty subset of V. Then D is a V if and only if every vector in V can be written as combination of elements of D over F in precisely one

field F basis of a linear way.

Proof: First, let us assume that D is a basis of V and that there exists an element v of V which can be written as a linear combination of elements of D over F in two different ways. That is to say, that there exists a finite } of D and there exist scalars a1 , . . . , an , b1 , . . . , bn in subset {v1 , . . . , vn n n for at least one F such that v = i=1 ai vi = i=1 bi vi , where n ah = bh n n index h. Then 0V = v − v = ( i=1 ai vi ) − ( i=1 bi vi ) = i=1 [ai − bi ]vi , where at least one of the scalars ai − bi is nonzero. This contradicts the assumption that D is a basis and hence linearly independent. Therefore every vector in V can be written as a linear combination of elements of D over F in precisely one way. Conversely, assume that every vector in V can be written as a linear combination of elements of D over F in precisely one way. That certainly implies that D is a generating set for V over F.If {v1 , . . . , vn } is a n . . . , an are scalars satisfying subset of D and if a1 , i=1 ai vi = 0V , then n n we have i=1 ai vi = i=1 0vi and so, by uniqueness of representation, we have ai = 0 for each 1 ≤ i ≤ n. This shows that D is linearly independent and so a basis.

58


We can look at Proposition 5.4 from another point of view. Let D be a nonempty subset of a vector space V over a field F, and define a function θ : F (D) → V by setting θ : f → u∈D f (u)u. (This sum is well-defined since only finitely-many of the summands are nonzero.) Then: (1) The function θ is monic if and only if D is linearly independent; (2) The function θ is epic if and only if D is a generating set; (3) The function θ is bijective if and only if D is a basis. (5.5) Proposition: Let D be a basis for a vector space V over a field F . Then any function f : D ×D → V can be extended in a unique manner to a function V × V → V which defines on V the structure of an F -algebra. Moreover, all F -algebra structures on V arise in this manner. Proof: Let D = {yi | i ∈ Ω}. Suppose that we are given a function f : D × D → V. We define an operation • on V as follows: if 5.4, we know that we can write v = v, w ∈ V, then, by Proposition a y and w = b y in a unique manner, where the ai i∈Ω i i j∈Ω j j and bj are scalars, only a finite number of which are nonzero; then set v • w = i∈Ω j∈Ω ai bj f (yi , yj ). It is straightforward to show that this defines the structure of an F -algebra on V. Conversely, if (V, •) is an F -algebra, define the function f : D × D → V by f : (yi , yj ) → yi • yj . The function f in Proposition 5.5 is the multiplication table of the vector multiplication operation •. Example: Let F be a field and let a, b ∈ F. Let B = {v1 , v2 , v3 , v4 } be the canonical basis for F 4 over F. Define an operation • on B according to the multiplication table: • v1 v2 v3 v4

v1 v1 v2 v3 v4

v2 v1 av1 −v4 −av3

v3 v3 v4 bv1 bv2

v4 v4 av3 −bv2 −abv1

4 4 and extend this operation to F 4 by setting i=1 ai vi • j=1 bj vj = 4 4 4 i=1 j=1 ai bj (vi • vj ). Then F , together with this operation, is a unital associative algebra known as a quaternion algebra over F, in which v1 is the identity element of for multiplication. In the special case of F = R and a = b = −1, we get the algebra of real quaternions, which is denoted by H. The algebra of real quaternions was first defined by Hamilton in 1844 as a generalization of the field of complex numbers (and earlier studied by Gauss, who did not publish his results). It is a division


59

algebra over R since every nonzero quaternion is a unit of H. These were subsequently generalized by Clifford and used in his study of noneuclidean spaces.2 Lately, they have also been used in computer graphics and in signal analysis. If F is a field having characteristic p > 0, quaternion algebras over F are not even entire. However, they arise naturally in the theory of elliptic curves, and so are of great importance in cryptography. If p > 2, then no quaternion algebras over F are commutative. We now show that any vector space over a field F has a basis. Indeed, the following two propositions show somewhat stronger than that3 . (5.6) Proposition: If V is a vector space finitely generated over a field F then every finite generating set of V over F contains a basis of V. Proof: Let V be a vector space finitely generated over a field F and let D be a finite generating set for V over F. If D is minimal among all generating sets for V, then we know by Proposition 5.2 that it is a basis of V. If not, it properly contains other generating sets for V over F, one of which, say E, has the fewest elements. Then E cannot properly contain any other generating set for V over F, and so it must be a basis of V.

2 Sir William Rowan Hamilton, a 19th-century Irish mathematician and physicist, helped create matrix theory in its modern formulation, together with Cayley and Sylvester. Hamilton was the first to use the terms “vector” and “scalar” in an algebraic context. His championship of quaternions as an alternative to vectors in physics was later taken up by Scottish mathematician Peter Guthrie Tait. Nineteenth-century British mathematician William Kingdom Clifford was one of the first to argue that energy and matter were just different types of curvature of space.

3

The Italian mathematician Giuseppe Peano, best known for his axiomatization of the natural numbers, was the first to prove that every finitelygenerated vector space has a basis at the end of the 19th century. He also gave the final form for the definition of a vector space, which we used above.

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(5.7) Proposition: If V is a vector space finitely generated over a field F then every linearly-independent subset B of V is contained in a basis of V over F. Proof: By assumption, there exists a finite generating set {v1 , . . . , vn } for V over F. Let B be a linearly-independent subset of V. If vi ∈ F B for each 1 ≤ i ≤ n, then F B = V, and B is itself a basis of V. Otherwise, / F B}. By Proposition 5.3, the set D = B ∪ {vh } let h = min{i | vi ∈ is linearly independent. If it is a generating set for V, then it is a basis / F D}, and replace D by and we are done. If not, let k = min{i | vi ∈ B ∪ {vh , vk }. Continuing in this manner, we see that after finitely-many steps we obtain a basis of V. We now want to extend this result to vector spaces which are not finitely generated, and to do so we have to make use of an axiom of set theory known variously as the Hausdorff Maximum Principle or Zorn’s Lemma4 . To state this principle, we need another concept about partially-ordered sets. Let A be a set on which we have defined a partial order . A subset B of A is bounded if and only if there exists an element a0 ∈ A satisfying b a0 for all b ∈ B. Note that we do not require that a0 belong to B. The Hausdorff maximum principle then says that if A is a partially-ordered set in which every chain subset is bounded, then A has a maximal element. Again, this is not really a “principle” or a “lemma”; it is an axiom of set theory which has been shown to be independent of the other (Zermelo-Fraenkel) axioms one usually assumes. Indeed, it is logically equivalent to the Axiom of Choice, which we mentioned in Chapter 1 as being somewhat controversial among those mathematicians dealing with the foundations of mathematics. However, in this book, we will assume that it holds. Given that assumption, we can now extend Proposition 5.7. (5.8) Proposition: If V is a vector space over a field F then every linearly-independent subset B of V is contained in a basis of V.

4 Felix Hausdorff, one of the leading mathematicians of the early 20th century and one of the founders of topology, died in a German concentration camp in 1942. Max Zorn, a German mathematician who emigrated to the United States, made skillful use of the Hausdorff Maximum Principle in his research, turning it into an important mathematical tool.


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Proof: Let B be a linearly-independent subset of V and let P be the collection of all linearly-independent subsets of V which contain B, which is partially-ordered by inclusion, as usual. Then P is nonempty since B ∈ P. Let Q be a chain subset of P. We want to prove that Q is bounded in P. That is to say, we want to find a linearly independent subset E of V which contains every element of Q. Indeed, let us take E to be the union of all of the elements of Q. To show that E is linearly independent, it suffices to show that every finite subset of E is linearly independent. Indeed, let {v1 , . . . , vn } be a finite subset of E. Then for each 1 ≤ i ≤ n, there exists an element Di of Q containing vi . Since Q is a chain, there exists an index h such that Di ⊆ Dh for all 1 ≤ i ≤ n and so vi ∈ Dh for all 1 ≤ i ≤ n. Therefore this set is a subset of a linearly-independent set and so is linearly independent. Thus we have shown that every chain subset of P is bounded and so, by the Hausdorff maximum principle, the set P has a maximal element. In other words, there exists a maximal linearly-independent subset of V containing B, and this, as we know, is a basis of V over F. Taking the special case of B = ∅ in Proposition 5.8, we see that every vector space has a basis. In the above proof we used the Axiom of Choice to prove this statement. In fact, one can show something considerably stronger: in the presence of the other generally-accepted axioms of set theory, the Axiom of Choice is equivalent, in the sense of formal logic, to the statement that every vector space over any field has a basis5 . Example: Consider the field R as a vector space over its subfield Q. A basis for this space is known as a Hamel basis. By Proposition 5.8, we know that Hamel bases exist, but nobody has been able to come up with a method of specifically constructing one. The subset C of R consisting of −i all real numbers which can be represented in the form i>0 ui 3 , where each ui is either 0 or 2, is called the Cantor set, and it can be shown to be “sparse” (in a technical sense of the word we won’t go into here) in the unit interval [0, 1] in R. It is possible to show that there is a Hamel basis of R contained in C. Still, the mere existence of Hamel bases leads to some very interesting results, as the following shows.

5

Andreas Blass.

This result is due to the contemporary American mathematician,

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Let H be a Hamel basis of R. If r ∈ R then we can write r = a∈H qa (r)a, where qa (r) ∈ Q and there are only finitely-many elements a ∈ H for which qa (r) = 0. Since such a representation is unique, we see that

1 if a = b qa (b) = 0 otherwise for a, b ∈ H. Moreover, if r, s ∈ R and a ∈ H then qa (r + s) = qa (r) + qa (s) so, if a = b are elements of H then for any r ∈ R we have qa (r + b) = qa (r) + qa (b) = qa (r). Thus we see that the function qa ∈ RR is periodic, with period b for any b ∈ H {a}, and its image is contained in Q. Moreover, if we pick two distinct elements c and d of H, we see that for each r ∈ R, we have r = f (r) + g(r), where f, g ∈ RR are defined by f : r → qc (r)c and g : r → a∈H{c} qa (r)a. By our previous comments, f is periodic with period d and g is periodic with period c. We conclude that the identity function in RR is the sum of two periodic functions. A somewhat more sophisticated argument along the same lines shows that any polynomial function in RR of degree n is the sum of n + 1 periodic functions. Of course, since we cannot specify H, there is no way of finding these periodic functions explicitly.6 We have seen that a vector space over a field can have many bases. We want to show next that if the vector space is finitely generated, then all of these bases are finite and have the same number of elements. First, however, we must prove a preliminary result. (5.9) Proposition: Let V be a vector space over a field F which is generated by a finite set B = {v1 , . . . , vn } and let D be a linearly independent set of vectors in V. Then the number of elements in D is at most n. Proof: Suppose that D has a subset E = {w1 , . . . , wn+1 } having more than n elements. Since this set must also be linearly independent, we know that none of the wi equals 0V . For each 1 ≤ k ≤ n, set Dk = {w1 , . . . , wk , vk+1 , . . . , vn }.

6 Twentieth-century German mathematician Georg Hamel was a student of Hilbert who worked primarily in function theory. In his later years, he became notorious for his pro-Nazi views and activities.


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Since B is a generating set for V, we can find scalars a1 , . . . , an , n not all equal to 0, such that w1 = i=1 ai vi . In order to simplify our notation, we will renumber elements of B if necessary so that a1 = 0. n the −1 w − a a vi and so D ⊆ F D1 . But D1 ⊆ V = F D Then v1 = a−1 1 i 1 i=2 1 and so V = F D1 by Proposition 3.6. Now assume that 1 ≤ k < n Then there exist scalars and that we have already shown that V = F Dk . k n b1 , . . . , bn , not all equal to 0, such that wk+1 = i=1 bi wi + i=k+1 bi vi . If the scalars bk+1 , . . . bn are all equal to 0, then we have shown that D is linearly dependent, which is not the case. Therefore at least one of them is nonzero and, by renumbering if necessary, we can assume that bk+1 = 0. k n −1 −1 Thus vk+1 = b−1 i=1 bk+1 bi wi − i=k+2 bk+1 bi vi and so, using k+1 wk+1 − the above reasoning, we get V = F Dk+1 . Continuing in this manner, we see that after n steps we obtain V = F Dn = F {w1 , . . . , wn }. But then wn+1 ∈ F {w1 , . . . , wn } and so E is linearly dependent, contrary to our assumption. This proves that D can have at most n elements. (5.10) Proposition: Let V be a vector space finitely generated over a field F. Then any two bases of V have the same number of elements. Proof: By hypothesis, there exists a finite generating set for V over F having, say, n elements. If B is a basis of V then, by Proposition 5.9, we know that B has at most n elements and so, in particular, is finite. Suppose B and B are two bases for V having h and k elements respectively. Since B is linearly independent and B is a generating set, we know that h ≤ k. But, on the other hand, B is linearly independent and B is a generating set, so k ≤ h. Thus h = k. We should remark at this point that the assertion for linearly-dependent sets corresponding to Proposition 5.10 is not true. That is to say, a finite linearly-dependent set of vectors may have two minimal linearly-dependent subsets with different numbers of elements. Indeed, there is no efficient algorithm to find such subsets of a given linearly-dependent set. We should also note that Proposition 5.9 is a special case of a more general theorem: if V is a vector space (not necessarily finitely generated) over a field F then there exists a bijective function between any two bases of V. The proof of this result makes use of techniques from advanced set theory, such as transfinite induction. If V is a vector space finitely generated over a field F then V is finite dimensional and the number of elements in a basis of V is called the dimension of V over F. If V is not finite dimensional, it is infinite dimensional. (In choosing this latter terminology, we are deliberately skipping over the subject of various transfinite dimensions, since the reader is not assumed to be familiar with the arithmetic of transfinite

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cardinals. In certain mathematical contexts, distinction between infinite dimensions – for example the distinction between spaces of countably-infinite and uncountably-infinite dimension – can be very significant. We will not, however, need it in this book.) We denote the dimension of V over F by dim(V ), or by dimF (V ) when it is important to emphasize the field of scalars7 . Notice that the proof of Proposition 5.9, which is in turn critical in proving Proposition 5.10, uses the fact that every nonzero element of F has a multiplicative inverse, and this cannot be avoided. If we try to weaken the notion of a vector space by allowing scalars to be, say, only integers, it may happen that such a space would have two bases of different sizes and so we could no longer define the notion of dimension in an obvious manner. We did not use, in an unavoidable manner, the commutativity of scalar multiplication and so we could weaken our notion of a vector space to allow scalars which do not commute among themselves, such as scalars coming from H. However, the generality thus gained does not seem to outweigh the bother it causes, and so we will refrain from doing so. Thus, for us, the fact that scalars always come from a field is critical in the development of our theory. Example: If F is a field then dim(F n ) = n for every positive integer n, since the canonical basis of F n has n elements. Similarly, if k and n are positive integers then dimF (Mk×n (F )) = kn, since the canonical basis of Mk×n (F ) has kn elements. The dimension of the space F [X] is infinite since the canonical basis of F [X] has infinitely-many elements. Example: If F is a field and n is a positive integer, then the set W of all polynomials in F [X] having degree at most n is a subspace of F [X] having dimension n + 1, since {1, X, . . . , X n } is a basis of W having n + 1 elements. Example: The dimension of R over itself is 1. Since {1, i} is clearly a basis of C as a vector space over R, we see that dimR (C) = 2 and so there cannot be a proper subfield F of C properly containing R.

7 The notion of dimension was implicit in the work of Peano, but was redefined and studied in a comprehensive manner by the 20th-century German mathematician Hermann Weyl.


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Indeed, if there were such a field, its dimension over R would have to be greater than 1 and less than 2 (else it would be equal to C), which is impossible. Clearly, dimR (H) = 4. It turns out that the only possible dimensions of division algebras over R are 1, 2, 4, and 8. The dimension 8 case is realized by a (non-associative) Cayley algebra over R, as defined in Chapter 15. There are no associative division algebras of dimension 8 over R.8 Example: Let F be a field, let (K, ∞•) bei an associative unital F algebra, and let v ∈ K. If p(X) = i=0 ai X ∈ F [X], then p(v) = ∞ i a v is an element of K and the set of all elements of K of this form i i=0 is an F -subalgebra of K, which is in fact commutative, even though K itself may not be. We will denote this algebra by F [v]. If the dimension of F [v], considered as a vector space over F, is finite, we know that there must exist a polynomial p(X) ∈ F [X] of positive degree satisfying p(v) = 0K . In that case, we say that v is algebraic over F. Otherwise, if the dimension of F [v] is infinite, we say v is transcendental over F. Thus, for example, the real numbers π and e (the base of the natural logarithms) are transcendental over Q. If F is a subfield of a field K then the set L of all elements of K which are algebraic over F is a subfield of K. Moreover, if K is algebraically closed, so is L, and in fact L is the smallest algebraically-closed subfield of K containing F. In particular, we can consider the field of all complex numbers algebraic over Q. This is a proper subfield of C, known as the field of algebraic numbers.9

8 Twentieth-century German mathematican Heinz Hopf used algebraic topology to prove that the only possible dimensions were powers of 2, and the final result was obtained by twentieth-century American mathematician Raoul Bott and contemporary American mathematician John Milnor, again using nonalgebraic tools.

9

The transcendence of π was proven by German mathematician Ferdinand von Lindemann in 1882. The transcendence of e was proven by French mathematician Charles Hermite in 1873. As we shall see later, Hermite made many important contributions to linear algebra.

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From the definition of dimension we see that if V is a vector space of finite dimension n over a field F then: (1) Every subset of V having more than n elements must be linearly dependent; (2) There exists a linearly-independent subset B of V having precisely n elements; (3) If B is as in (2) then B is also a generating set of V over F. (5.11) Proposition: Let V be a vector space finitely generated over a field F and let W be a subspace of V. Then: (1) W is finitely generated over F ; (2) Every basis of W can be extended to a basis of V ; (3) dim(W ) ≤ dim(V ), with equality when and only when W = V. Proof: Let n = dim(V ). (1) If W is not finitely generated, then, as we remarked after Proposition 5.3, W has a linearly-independent subset B having n + 1 elements. But B is also a subset of V, contradicting the assumption that dim(V ) = n. (2) Let B be a basis of W. Then B is as linearly-independent set of elements of V and so, by Proposition 5.7, can be extended to a basis of V. (3) By (2), we see that the number of elements of a basis of W can be no greater than the number of elements of a basis of V, and so dim(W ) ≤ dim(V ). Moreover, if we have equality then any basis B of W is also a basis of V, and so W = F B = V. We now want to extend the notion of linear independence. Let U and W be subspaces of a vector space V over a field F. Any vector v ∈ U +W can be written in the form u + w, where u ∈ U and w ∈ W, but there is no reason for this representation to be unique. It will be unique, however, if U and W are disjoint. Indeed, if this condition holds and if u, u ∈ U and w, w ∈ W satisfy u + w = u + w , then u − u = w − w ∈ U ∩ W and so u − u = 0V = w − w , which in turn implies that u = u and w = w . To emphasize the importance of this situation, we will introduce new notation: if U and W are disjoint subspaces of a vector space V over a field F, we will write U ⊕ W instead of U + W. The subspace U ⊕ W is called the direct sum of U and W . We note that, by this definition, U ⊕ {0V } = U for every subspace U of V. ! ! 1 0 2 ⊕R . Example: It is easy to see that R = R 0 1 Of course, we would like to extend the notion of direct sum to cover more than two subspaces. In general, if V is a vector space over a field F ,


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then a collection {Wh | h ∈ Ω} of subspaces of V is independent if and only if it satisfies the following condition: if Λ is a finite subset of Ω and if we choose elements wh ∈ Wh for all h ∈ Λ, then h∈Λ wh = 0V when and only when wh = 0V for each h ∈ Λ. Thus we see that an infinite collection of subspaces is independent if and only if every finite nonempty subcollection is independent. Clearly, a subset D of a vector space V over a field F is linearly independent if and only if the collection of subspaces {F v | v ∈ D} is independent. (5.12) Proposition: Let V be a vector space over a field F and let W1 , . . . , Wn be distinct subspaces of V. Then the following conditions are equivalent: (1) {W1 , . . . Wn } is independent; n (2) Every vector w ∈ i=1 Wi can be written as w1 + . . . + wn , with wi ∈ Wi for each 1 ≤ i ≤ n, in exactly one way; (3) Wh and i=h Wi are disjoint, for each 1 ≤ h ≤ n. n Proof: (1) ⇒ (2): Let w ∈ i=1 Wi and assume that we can write + . . . + wn = y1 + . . . + yn , where wi , yi ∈ Wi for each 1 ≤ i ≤ n. w = w1 n Then i=1 (wi − yi ) = 0V and so, by (1), it follows that wi − yi = 0V for each 1 ≤ i ≤ n, proving (2). (2) ⇒ (3): Assume that 0V = wh ∈ Wh ∩ i=h W i . Then for each i = h there exists an element wi ∈ Wi satisfying wh = i=h wi , contradicting (2). (3) ⇒ (1): Suppose we can write w1 + . . . + wn = 0V , where wi ∈ Wi foreach 1 ≤ i ≤ n, and where wh = 0V for some h. Then wh = − i=h wi ∈ Wh ∩ i=h Wi , and this contradicts (3). Thus (1) must hold. If V is a vector space over a field F and if {W , i | i ∈ Ω} is an independent collection of subspaces of V, we write i∈Ω Wi instead of W . If Ω = {1, . . . , n}, we will also write this sum as W1 ⊕. . .⊕Wn . i i∈Ω , If V = i∈Ω Wi , then we say that V has a direct-sum decomposition relative to the subspaces Wi . Example: If B is a basis of a vector space V over a field F then , V = v∈B F v. The importance of direct-sum decompositions is illustrated by the following result. (5.13) Proposition: Let V be a vector space over a field F , let {Wi | i ∈ Ω} be a pairwise disjoint collection of subspaces , of V and, for each i ∈ Ω, let Bi be a basis of Wi . Then V = i∈Ω Wi if and only if B = i∈Ω Bi is a basis of V.

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, Proof: Assume V = i∈Ω Wi and,let v ∈ V. Then there exists a Wi , and so for each i ∈ Λ finite subset Λ of Ω such that v ∈ i∈Λ there is an element wi ∈ Wi satisfying v = i∈Λ wi . Moreover, each wi is a linear combination of elements of Bi . Thus v is a linear combination of elements of B, and so B is a generating set for V. We are left to show that B is linearly independent. If that is not the case, then there exist an element h of Ω, vectors y1 , . . . , yt in B h , and scalars a1 , . . . , at in t F, not all of which equal to 0, such that j=1 aj vj + u = 0V , where t u is a linear combination of elements of i=h Bi . But then j=1 aj vj ∈ our initial assumption. Thus B = Wh ∩ i=h Wi , contradicting i∈Ω Bi . Conversely, if B = i∈Ω Bi , itthen follows that every element of V can be written in a unique way as i , where Λ is some finite subset i∈Λ w , of Ω, which suffices to prove that V = i∈Ω Wi . Let W be a subspace of a vector space V over a field F. A subspace Y of V is a complement of W in V if and only if V = W ⊕ Y. We immediately note that if Y is a complement of W in V then W is a complement of Y in V. In general, a subspace of a vector space can have many complements. Example: Each of the following subspaces of R2 is a complement of each of the others in R2 :

!

! a 0 W1 = a ∈ R ; W2 = b∈R ; 0 b

!

! c d W3 = c ∈ R ; and W4 = d∈R . c 2d (5.14) Proposition: Every subspace W of a vector space V over a field F has at least one complement in V. Proof: If W is improper, then {0V } is a complement of W in V. Similarly, V is a complement of {0V } in V. Otherwise, let B be a basis of W. By Proposition 5.8, we know that there exists a linearlyindependent subset D of V such that B ∪ D is a basis of V. Then F D is a complement of W in V. Example: Let F be a field of characteristic other than 2, let n be a positive integer, and let V be a vector space over F. Let W = Mn×n (V ), which is also a vector space over F. Let W1 be the set of all those matrices A = [vij ] in W satisfying vij = vji for all 1 ≤ i, j ≤ n, and let W2 be the set of all those matrices A = [vij ] in W satisfying vij = −vji for all 1 ≤ i, j ≤ n. These two subspaces are disjoint. If A = [vij ] is an arbitrary matrix in W, then we can write A = B + C, where B = [yij ]


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is the matrix defined by yij = 12 (vij + vji ) for all 1 ≤ i, j ≤ n, and C = [zij ] is the matrix defined by zij = 12 (vij − vji ) for all 1 ≤ i, j ≤ n. Note that A ∈ W1 and B ∈ W2 . Thus V = W1 ⊕ W2 . Example: A function f ∈ RR is even if and only if f (a) = f (−a) for all a ∈ R; it is odd if and only if f (a) = −f (−a) for all a ∈ R. The set W of all even functions is clearly a subspace of RR , as is the set Y of all odd functions, and these two subspaces are disjoint. Moreover, if f ∈ RR then f = f1 + f2 , where the function f1 : x → 12 [f (x) + f (−x)] is in W and the function f2 : x → 12 [f (x) − f (−x)] is in Y. Thus Y is a complement of W in RR . (5.15) Proposition: Let F be a field which is not finite and let V be a vector space over F having dimension at least 2. Then every proper nontrivial subspace W of V has infinitely-many complements in V. Proof: By Proposition 5.14 we know that W has at least one complement U in V. Choose a basis B for U. If 0V = w ∈ W, then by Proposition 3.2(9) and the fact that F is infinite, we know that F w is an infinite subset of W. Thus we know that the set W is infinite. For each w ∈ W, let Yw = F {u + w | u ∈ B}. We claim that each of these spaces is a complement of W in V. Indeed, assume that v ∈ W ∩ Yw . Then there exist elements n u1 , . . . , un of B , . . . , c in F satisfying v = and scalars c 1 n i=1 ci (ui + w). But n n c u = v − ( c ) w ∈ W ∩ U = {0 then V } and since the set i=1 i i i=1 i {u1 , . . . , un } is linearly independent, we see that ci = 0 for all i. This shows that v = 0V , and we have thus shown that W and nYw are disjoint. If v is an arbitrary element of V, let us write v = x+( i=1 ci ui ) , where belong to B,and the scalars c1 , . . . , cn x ∈ W , the vectors u1 , . . . , un n n belong to F. Then v = [x − ( i=1 ci ) w] + i=1 ci (ui + w) ∈ W + Yw and thus we have shown that V = W + Yw and so Yw is a complement of W in V. We are left to show that all of these complements are indeed different from each other. Indeed, assume that w = x are elements of W satisfying Yw = Yx . If u ∈ B then there exist n elements u1 , . . . , un of B and scalars . . , cn such that u + w = c1 , . i=1 ci (ui + x). From this it follows that n n u − i=1 ci ui = ( i=1 ci ) x − w and this belongs to W ∩ Yw = {0V }. But B is a linearly-independent set and so u has to equal to one of the uh for some 1 ≤ h ≤ n, and we must have ci = 0 for i = h and ch = 1. Hence x − w = 0V , namely x = w. This is a contradiction, and so the Yw must all be distinct. (5.16) Proposition (Grassmann’s Theorem): Let V be a vector space over a field F and let W and Y be subspaces of V

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satisfying the condition that W + Y is finite-dimensional. Then dim(W + Y ) = dim(W ) + dim(Y ) − dim(W ∩ Y ). Proof: Let U0 = W ∩Y, which is as subspace both of W and of Y. In particular, U0 has a complement U1 in W and a complement U2 in Y. Then W +Y = U0 +U1 +U2 . We claim that in fact W +Y = U0 ⊕U1 ⊕U2 . Indeed, assume that u0 + u1 + u2 = 0V , where uj ∈ Uj for j = 0, 1, 2. Then u1 = −u2 − u0 ∈ W ∩ Y = U0 . But U0 and U1 are disjoint and so u1 = 0V . Therefore u0 = −u2 ∈ U0 ∩ U2 = {0V }. Therefore u0 = 0V and u2 = 0V as well. Thus we see that the set {U0 , U1 , U2 } is independent. Therefore, from the definition of the complement, we have dim(W + Y ) = dim(U0 ) + dim(U1 ) + dim(U2 ) = dim(W ) + dim(U2 ) and this equals dim(W ) + dim(Y ) − dim(W ∩ Y ) since Y = U2 ⊕ (W ∩ Y ).     1   1 and Example: Consider the subspaces W1 = R  0  ,  2    2 2     0   1 W2 = R  1  ,  1  of R3 . Each one of these subspaces has   0 1 dimension 2, and so we see that 2 ≤ dim(W1 + W2 ) ≤ 3. By Proposition 5.16, we see that, as a result of this, we have 1 ≤ dim(W1 ∩ W2 ) ≤ 2. In order to ascertain the exact dimension of W1 ∩ W2 we must find a basis for it. If v ∈ W1 ∩ W2 then there exist scalars a, b, c, d satisfying         1 1 1 0 a  0  + b  2  = c  1  + d  1  , and so a + b = c, 2b = c + d, 2 2 0 1 and 2a + 2b = d, from which we conclude that  b = −3a, c = −2a, and    1 0 d = −4a. Thus v has to be of the form (−2a)  1  + (−4a)  1  = 0 1     −2 −2 a  −6  , which shows that W1 ∩ W2 = R  −6  , and so it has −4 −4 dimension 1.


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Exercises Exercise 131 Let v1 , v2 , and v3 be elements of a vector space V over a field F and let c1 , c2 , c3 ∈ F. Is the subset {c2 v3 − c3 v2 , c1 v2 − c2 v1 , c3 v1 − c1 v3 } of V necessarily linearly dependent? Exercise 132 For which values of the real number t is the subset

! !cos(t) + i sin(t) 1 , 1 cos(t) − i sin(t) of C2 linearly dependent? Exercise 133 Consider the functions f : x → 5x and g : x → 52x . Is {f, g} a linearly-dependent subset of RR ?     2 a    a − b , b  Exercise 134 Find a, b ∈ Q such that the subset   1 3 of Q3 is linearly dependent. Exercise 135 Let V be a vector space over a field F and let n > 1 be   v1   an integer. Let Y be the set of all vectors  ...  ∈ V n satisfying the vn condition that the set {v1 , . . . .vn } is linearly dependent. Is Y necessarily a subspace of V n ?       1+i  1−i  1+i  3 + 8i  ,  5  ,  3 + 2i  of Exercise 136 Is the subset   4−i 2+i 5 + 7i C3 linearly independent, when we consider C3 as a vector space over C? Is it linearly independent when we consider C3 as a vector space over R? Exercise 137 For each nonnegative integer n, let fn ∈ RR be the function defined by fn : x → sinn (x). Is the subset {fn | n ≥ 0} of RR linearly independent? Exercise 138 Let V = C(−1, 1), which is a vector space over R. Let f, g ∈ V be the functions defined by f : x → x2 and g : x → |x|x. Is {f, g} linearly independent?

72


Exercise 139 Let V be a vector space over GF (5) and let v1 , v2 , v3 ∈ V. Is the subset {v1 + v2 , v1 − v2 + v3 , 2v2 + v3 , v2 + v3 } of V linearly independent? Exercise 140 Let F be a field of characteristic different from 2 and let V be a vector space over F containing a linearly-independent subset {v1 , v2 , v3 }. Show that the set {v1 + v2 , v2 + v3 , v1 + v3 } is also linearly independent.         1 1 1 0          1   2  1 2         Exercise 141 Is the subset   ,  , , of GF (3)4 2 1   1   2       2 2 2 0 linearly independent? Exercise 142 Let t ≤ n be positive integers and, for all 1 ≤ i ≤ t, let   ai1 t   vi =  ...  be a vector in Rn chosen so that 2|ajj | > i=1 |aij | for ain all 1 ≤ j ≤ n. Show that is linearly independent. Exercise 143 If {v1 , v2 , v3 , v4 } is a linearly-independent subset of a vector space V over the field Q, is the set {3v1 + 2v2 + v3 + v4 , 2v1 + 5v2 , 3v3 + 2v4 , 3v1 + 4v2 + 2v3 + 3v4 } linearly independent as well? Exercise 144 Let A be a subset of R having at least three elements and let f1 , f2 , f3 ∈ RA be the functions defined by fi : x → xi−1 2x−1 . Is the set {f1 , f2 , f3 } linearly independent? Exercise 145 Let F = GF (5) and let V = F F , which is a vector space over F. Let f : x → x2 and g : x → x3 be elements of V. Find an element h of V such that {f, g, h} is linearly independent. Exercise 146 Consider R as a vector space over Q. . / (a − π)−1 | a ∈ Q of this space linearly independent?

Is the subset

Exercise 147 In the vector space V = RR over R, consider the functions 2 (x + 1)3 f1 : x → ln , x4 + 7 √ f2 : x → ln x2 + 1 , and f3 : x → ln x4 + 7 . Is the subset {f1 , f2 , f3 } of V linearly independent?

5. Linear  independence and dimension 

73

       0 2   1  Exercise 148 Show that the subset  2  ,  1  ,  0  of GF (p)3    0 2 1  is linearly independent if and only if p = 3. Exercise 149 Let F be a subfield of a field K and let n be a positive integer. Show that a nonempty linearly-independent subset D of F n remains linearly independent when considered as a subset of K n . Exercise 150 Let F = GF (5) and let V = F F . For 4 ≤ k ≤ 7, let fk ∈ V be defined by fk : a → ak . Is the subset {fk | 4 ≤ k ≤ 7} of V linearly independent? Exercise 151 Let V be a vector space over R. For vectors v = w in V, let K(v, w) be the set of all vectors in V of the form (1 − a)v + aw, where 0 ≤ a ≤ 1. Given vectors v, w, y ∈ V satisfying the condition that the set {w − v, y − v} is linearly independent (and so, in particular, its elements are distinct), show that the set K(v, 12 (w + y)) ∩ K(w, 12 (v + y)) ∩ K(y, 12 (v + w)) is nonempty, and determine how many elements it can have. Exercise 152 Let V be a vector space finitely generated over a field F and let B = {v1 , . . . , vn } be a basis for V. Let y ∈ V B. Show that the set {v1 , . . . , vn , y} has a unique minimal linearly-dependent subset. Exercise 153 Find all of the minimal linearly-dependent subsets of the

! ! ! ! !1 0 0 2 2 subset , , , , of Q2 . 0 4 0 0 2 Exercise 154 Let F be a field of characteristic other than 2. Let V be the / polynomials of degree at most 3. . subspace of F [X] consisting of all Is X + 2, X 2 + 1, X 3 + X 2 , X 3 − X 2 a basis of V ? Exercise 155 Let {v1 , . . . , vn } be a basis for a vector space V over a field F. Is the set {v1 + v2 , v2 + v3 , . . . , vn−1 + vn , vn + v1 } necessarily also a basis for V over F ? √ √ √ Exercise 156 Is {1 + 2 5, − 3 + 5} a basis for Q( 5) as a vector space over Q? Exercise 157 For which values of a ∈ R is the set

! ! ! a 2a 1 2 1 2a 1 , , , 2 3a 2a 3 a+1 a+2 2 a basis for M2×2 (R) as a vector space over R?

a+1 2a = 1

!-

74


Exercise 158 Let A be a nonempty finite set and let P be the collection of all subsets of A. Let F be a field and let K be the vector space over operation • on K by setting B | B ∈ P }. Define Fhaving basis {v an • = a v d v B B C C B∈P C∈P B∈P C∈P aB dC vB∪C . Is K an F -algebra? If so, is it associative? Exercise 159 Let F be an algebraically-closed field and let (K, •) be an associative F -algebra having a basis {v1 , v2 } as a vector space over F. Show that v22 = v2 or v22 = 0K . Exercise 160 Find a basis for the subspace W of        4 1 1 1      −1   2   5 2         6  ,  3  ,  0  ,  −3    −2 −1 0 1

R4 generated by      .   

Exercise 161 For each real number a, let fa ∈ RR be defined by

1 if r = a fa : r → . 0 otherwise Is {fa | a ∈ R} a basis for RR over R? Exercise 162 Let A be a nonempty finite set and let V be the collection of all subsets of A, which is a vector space over GF (2). For each a ∈ A, let va = {a}. Is {va | a ∈ A} a basis for V ? Exercise 163 Let F be a field and let a, b, c ∈ F. Determine whether       0 0  1   a , 1 ,  0 is a basis for F 3 .   b c a+b+c Exercise 164 Let V be a vector finitely generated1over a field F 0 space 2 n having a basis {v1 , . . . , vn }. Is v1 , i=1 vi , . . . , i=1 vi necessarily a basis for V ? Exercise 165 Let F = GF (p) for some prime integer p, let n be a positive integer, and let V be a vector space of dimension n over F. In how many ways can we choose a basis for V ? Exercise 166 Let V be a three-dimensional vector space over a field F, with basis {v1 , v2 , v3 }. Is {v1 + v2 , v2 + v3 , v1 − v3 } a basis for V ? Exercise 167 Let V be a vector space of finite dimension n over C having basis {v1 , . . . , vn }. Show that {v1 , . . . , vn , iv1 , . . . , ivn } is a basis for V, considered as a vector space over R. Exercise 168 Let V be a vector space of finite dimension n > 0 over R and, for eachpositive integer i, let Ui be a proper subspace of V. ∞ Show that V = i=1 Ui .


75

Exercise 169 Let V be a vector space over a field F which is not finite dimensional, and let W be a proper subspace of V. Show that there exists an infinite collection {Y1 , Y2 , . . .} of subspaces of V satisfying n ∞ Y ⊆ W but Y W for all n ≥ 1. i i i=1 i=1 Exercise 170 Let V be the subspace of R[X] consisting of all polynomials of degree at most 5, and let A = {X 5 +X 4 , X 5 −7X 3 , X 5 −1, X 5 +3X}. Show that this subset of V is linearly independent and extend it to a basis of V. Exercise 171 Let V be a vector space of finite dimension n over a field F, and let W be a subspace of V of dimension n − 1. If U is a subspace of V not contained in W, show that dim(W ∩ U ) = dim(U ) − 1. Exercise 172 Let a, b, c, d be rational numbers such that √ √ {a + c 3, b + d 3} √ √ √ is a basis for √ Q( 3) as a vector space over Q. Is {c +√a 3, d + √b 3} a basis for Q( √ 3) as a vector space over Q? Is {a + c 5, b + d 5} a basis for Q( 5) as a vector space over Q? Exercise 173 Find a real number a such that            −9 2 1 3 −1                 a      −5   4   −1   9             dim R  −1  ,  3  ,  −1  ,  2  ,  −4    = 2.      −5   0   1   1   1         −14 2 2 4 0        2 1 −1           1  1 2       Exercise 174 Let W = R   ,  , ⊆ R4 . Determine 3 0   −3        1 1 0  the dimension of W and find a basis for it.    Exercise 175 Consider the vectors v1 =         

0 3 0 4 0





     , v4 =     

1 9 5 7 1





     , and v5 =     

0 1 0 5 0



0 1 0 1 0





     , v2 =     

7 4 1 8 3

    , v3 =  

   in the vector space Q5 . Do  

there exist rational numbers aij , for 1 ≤ i, j ≤ 5, such that the subset 0 1 5 of Q5 is linearly independent? j=1 aij vj 1 ≤ i ≤ 5

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Exercise 176 Let F be a subfield of a field K satisfying the condition that K is finitely generated as a vector space over F. For each c ∈ K, show that there exists a nonzero polynomial p(X) ∈ F [X] satisfying p(c) = 0.     1 −1       1  2      Exercise 177 Let W = R  , ⊆ R4 and let V = 1   1       0 1     2 −5        6  −1     R  , . Compute dim(W + V ) and dim(W ∩ V ). 0   3       1 0 Exercise 178 Let F be a subfield of a field K satisfying the condition that the dimension of K as a vector space over F is finite and equal to r. Let V be a vector space of finite dimension n > 0 over K. Find the dimension of V as a vector space over F. Exercise 179 Let V be a vector space over a field F having infinite dimension over F. Show that there exists a countably-infinite collection of proper subspaces of V, the union of which equals V. Exercise 180 Let F = GF (p), where p is a prime integer, and let V be a vector space over F having finite dimension n. How many subspaces of dimension 1 does V have? Exercise 181 Let W be the subset of RR consisting of all functions of the form x → a · cos(x − b), for real numbers a and b. Show that W is a subspace of RR and find its dimension.       4 6 1          3   2   ,  1  ⊆ R4 and let Y = Exercise 182 Let W = R  ,  2   2   1       1 2 2     4 1        0  −2 ,  ⊆ R4 . Find dim(W + Y ) and dim(W ∩ Y ). R   0   3       −2 2 Exercise 183 Let V be a vector space of finite dimension n over a field F and let W and Y be distinct subspaces of V, each of dimension n − 1. What is dim(W ∩ Y )? Exercise 184 Let V be a finite-dimensional vector space over a field F and let B be a basis of V satisfying the condition that


w w

77

! w∈B

is a basis for V 2 . What is the dimension of V ? Exercise 185 Let F be a field and let V be the subspace of F [X] consisting of all polynomials of degree at most 4. Find a complement for V in F [X]. Exercise 186 Let F be a field and let V be the subspace of F [X] consisting of all polynomials of the form (X 3 + X + 1)p(X) for some p(X) ∈ F [X]. Find a complement for V in F [X]. Exercise 187 Let B be a nonempty proper subset of a set A. Let F be a field and let V = F A . Let W be the subspace of V consisting of all those functions f ∈ V satisfying f (b) = 0 for all b ∈ B. Find a complement of W in V. Exercise 188 Let F be a field of characteristic other than 2, let V be a    v   vector space over F, and let U =  v  v, v ∈ V ⊆ V 3 . Is   v + v     v  Y =  v  v ∈ V a complement of U in V ?   v Exercise 189 Let F be a field and let p(X) ∈ F [X] have positive degree k. Let W be the subspace of F [X] composed of all polynomials of the form p(X)g(X) for some g(X) ∈ F [X]. Show that W has a complement in F [X] of dimension k. Exercise 190 Let V be a vector space over a field F which is not finite dimensional, and let V ⊃ W1 ⊃ W2 ⊃ . . . be a chain of subspaces ∞ of V, each properly contained in the one before it. Is the subspace i=1 Wi of V necessarily finite-dimensional? Exercise 191 Let V be a vector space finite dimensional over a field F. Let W and Y be subspaces of V and assume that there is a function f ∈ F V satisfying the condition that f (w) < f (y) for all 0V = w ∈ W and 0V = y ∈ Y. Show that dim(W ) + dim(Y ) ≤ dim(V ). Exercise 192 Let (K, •) be a division algebra of dimension 2 over R containing an element v1 which satisfies the condition that v1 • v = v = v • v1 for all v ∈ V. Show that (K, +, •) is a field. Exercise 193 For each a ∈ R, the set Q[a] = {p(a) | p(X) ∈ Q[X]} is a subspace of R, considered as a vector space over Q. Find all pairs (a, b)

78


of real numbers a = b satisfying the condition that the set {Q[a], Q[b]} is independent over Q. Exercise 194 Let V be a vector space over a field F. Find a necessary and sufficient condition for there to exist subspaces W and W of V such that {{0V }, W, W } is independent. Exercise 195 Let (K, •) be a unital R-algebra (not necessarily associative) with multiplicative identity e, and let {vi | i ∈ Ω} be a basis for K over R containing e (which isequal to vt for some t ∈ Ω). If v = i∈Ω ci vi ∈ K, set v = ct vt − i=t ci vi . If v ∈ K, is it true that vv = vv and v = v? (Note that this construction generalizes the notion of the conjugate of a complex number.) Exercise 196 For each nonnegative integer n, define the subsets Pn , An , and Fn of R as follows: (1) P0 = ∅, A0 = {1}, and F0 = Q; (2) If n > 0, then Pn is the set of the first n prime integers, An consists of 1 and the set of square roots of products of distinct elements of Pn , and Fn = QAn . Show that each An is a linearly-independent subset of R, considered as a vector space over Q, and that Fn is a subfield of R, having the property that every element of Fn the square of which belongs to Q must belong to Qa, for some a ∈ An .

6 Linear transformations

Let V and W be vector spaces over a field F. A function α : V → W is a linear transformation1 or homomorphism if and only if for all v1 , v2 ∈ V and a ∈ F we have α(v1 + v2 ) = α(v1 ) + α(v2 ) and α(av1 ) = aα(v1 ). We note that, as a consequence of the second condition, we have α(0V ) = α(00V ) = 0α(0V ) = 0W . If (K, •) and (L, ∗) are F algebras, then a linear transformation α : K → L is a homomorphism of F -algebras if it is a linear transformation and, in addition, satisfies α(v1 • v2 ) = α(v1 ) ∗ α(v2 ) for all v1 , v2 ∈ K. If both K and L are unital, then it is a homomorphism of unital F -algebras if it also sends the identity element of K for • to the identity element of L for ∗. Example: Let V be a vector space over a field F. Every scalar c ∈ F defines a linear transformation σ c : V → V given by σ c : v → cv. In

1 Linear transformations between finite-dimensional vector spaces were studied by Peano. Linear transformations between infinite-dimensional spaces were first considered in the late 19th century by Italian mathematician Salvadore Pincherle.

79

80

6. Linear transformations

particular, σ 1 is the identity function v → v and σ 0 is the 0-function v → 0V . Example: Let F be a field and let a1 , . . . , a6 be scalars in F. The   ! a1 c1 + a2 c2 c1 →  a3 c1 + a4 c2  is a function α : F 2 → F 3 defined by α : c2 a5 c1 + a6 c2 linear transformation. The previous example can be generalized in an extremely significant manner. Let k and n be positive integers and let F be a field. Every matrix A = [aij ] ∈ Mk×n (F ) defines a linear transformation from F n     c1 a11 c1 + . . . + a1n cn  c2   a21 c1 + . . . + a2n cn      to F k given by  .  →   . In what follows, ..  ..    . cn ak1 c1 + . . . + akn cn we will show that every linear transformation from F n to F k can be defined in this manner. Example: Let F be a field of characteristic 0. Then there are linear transformations α and β from F [X] to itself defined by α:

∞

ai X i →

i=0

∞

iai X i

i=0

and β :

∞

ai X i →

i=0

∞ (1 + i)−1 ai X i+1 . i=0

(By 1 + i, we mean the sum of 1 + i copies of the identity element for multiplication of F ; since the characteristic of F is 0, we know that this element is nonzero, and so is a unit in F.) Example: Let V and W be vector spaces over a field F and let k and n be positive integers. For all 1 ≤ i ≤ k and 1 ≤ j ≤ n, let αij : V → W be a linear transformation. Then there is a linear transformation from Mk×n (V ) to Mk×n (W ) defined by     v11 . . . v1n α11 (v11 ) . . . α1n (v1n )   .. .. .. ..  →  .  .  . . .  vk1

...

vkn

αk1 (vk1 )

...

αkn (vkn )

Example: Let V be the subspace over RR consisting of all differentiable functions. For each f ∈ V, we define a function Df : R × R → R, called the differential of f, by setting Df : (a, b) → f (a)b, where f is the derivative of f. Then the function D : V → RR×R given by f → Df


81

is a linear transformation. These linear transformations play an important part in differential geometry. Example: Linear transformations are considered nice from an algebraic point of view, but may be less so from an analytic point of view. Let B be a Hamel basis of R over Q. Then for each real number r there exists a unique finite subset {u1 (r), . . . , un(r) (r)} of B and scalars n(r) a1 (r), . . . , an(r) (r) in Q satisfying r = j=1 aj (r)uj (r). The function n(r) from R to R defined by r → j=1 aj (r) is a linear transformation, but is not continuous at any r ∈ R. Let V

and W

be vector spaces over a field F. To any function

! v v∈V f : V → W can associate the subset gr(f ) = f (v) of V × W , called the graph of f. We can use the notion of graph to characterize linear transformations in terms of subspaces. (6.1) Proposition: Let V and W be vector spaces over a field F and let α : V → W be a function. Then α is a linear transformation if and only if gr(α) is a subspace of V × W. Proof: Assume that α is a linear transformation. If v, v ∈ V c ∈ F then in V × W we have v α(v) and c

! +

v α(v)

v α(v )

! =

!

v + v α(v) + α(v )

=

cv cα(v)

! =

cv α(cv)

! =

v + v α(v + v )

and

! ∈ gr(α)

! ∈ gr(α), showing that gr(α)

is closed under taking sums and scalar multiples, and so is a subspace of V × W . Conversely, if it is such a subspace then for v, v ∈ V and c ∈ F ! ! ! v + v v v = ∈ gr(α) and we note that + α(v ) α(v) + α(v ) α(v) ! v = so we must have α(v) + α(v ) = α(v + v ). Similarly, c α(v) ! cv ∈ gr(α) and so we must have cα(v) = α(cv). Thus α is a cα(v) linear transformation. Let V and W be vector spaces over a field F. If α and β be linear transformations from V to W, they are, in particular, functions in W V

82


and so the function α + β : V → W is defined by α + β : v → α(v) + β(v) for all v ∈ V. For all v, v ∈ V and all c ∈ F we have (α + β)(v + v )

= α(v + v ) + β(v + v ) = α(v) + α(v ) + β(v) + β(v ) =

(α + β)(v) + (α + β)(v ).

and (α + β)(cv) = α(cv) + β(cv) = cα(v) + cβ(v) = c[α(v) + β(v)] = c(α + β)(v). Thus we see that α + β is a linear transformation from V to W. If c ∈ F is a scalar then the function cα from V to W is defined by cα : v → cα(v) and this, again, is a linear transformation from V to W. It is easy to check that the set of all linear transformations from V to W is a subspace of W V , which we will denote by Hom(V, W ). This means that we can apply concepts we have already considered for vectors to linear transformations. For example, we can talk about a linearly-dependent or linearly-independent set of linear transformations from a vector space V over a field F to a vector space W over F . However, we must be very careful to remember that when we are doing so, we are working in the space Hom(V, W ), and not in either V or W. The following example illustrates the pitfalls one can encounter. Example: Let V and W be vector spaces over the same field F. A nonempty subset D = {α1 , . . . , αn } of Hom(V, W ) is locally linearly dependent if and only if the subset {α1 (v), . . . , αn (v)} of W is linearly dependent for every v ∈ V. If D is a linearly-dependent subset of Hom(V, W ), then there n exist scalars c1 , . . . , cn , not all of which are equal to 0, such that i=1 nci αi is the 0-function. In particular, for each v ∈ V we see that i=1 ci αi (v) = 0W and so D is locally linearly dependent. The converse, however, is false. It may be possible for D to be linearly independent and still locally linearly dependent. To see this, take V = W = F 2 and let D = {α1 , α2 } ⊆ Hom(F 2 , F 2 ), where we ! ! ! ! a a a b define α1 : → and α2 : → . If v ∈ F 2 , then b 0 b 0 ! 1 of {α1 (v), α2 (v)} is a subset of the one-dimensional subspace F 0 F 2 and so cannot be linearly independent. On the other hand, D is linearly independent since if there exist scalars c and d satisfying the condition that cα1 + dα2 is the 0-function, then ! ! ! ! ! ! 1 1 c 0 c 0 + dα2 = + = , = cα1 0 0 0 0 0 0 which implies that c = 0. Similarly, ! ! ! 0 0 0 = cα1 + dα2 = 0 1 1

0 0

! +

0 d

! =

0 d

! ,


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which implies that d = 0 as well. The following proposition shows that the operation of a linear transformation is entirely determined by its action on elements of a basis. This result is extremely important, especially if the vector spaces involved are finitely generated. (6.2) Proposition: Let V and W be vector spaces over a field F, and let B be a basis of V. If f ∈ W B then there is a unique linear transformation α ∈ Hom(V, W ) satisfying the condition that α(u) = f (u) for all u ∈ B. Proof: Since B is a basis of V, we know n that each vector v ∈ V can be written as a linear combination v = i=1 ai ui of elements of B in na unique way. We now define the function α : V → W by α : v → i=1 ai f (ui ). This function is well defined as a result of the uniqueness of representation of v, as was shown in Proposition 5.4. Moreover, it is clear that α is a linear transformation. If β : V → W is a linear transformation satisfying the condition that β(u) n n = f (u) for all u ∈ B n then β(v) = β ( i=1 ai ui ) = i=1 ai β(ui ) = i=1 ai f (ui ) = α(v) and so β = α. Thus α is unique. Example: We can use Proposition 6.2 to show how uncommon linear transformations really are. Let F = GF (3) and let V = F 4 . Then V has 34 = 81 elements and so the number of functions from V to itself is 8181 . On the other hand, a basis B for V over F has 4 elements and so, since every linear transformation from V to itself is totally determined by its action on B and that any function from B to V defines such a linear transformation, we see that the number of linear transformations from V to itself is 814 . Therefore, the probability that a randomly-selected function from V to itself is a linear transformation is 814 /8181 = 81−77 , which is roughly 0.11134 × 10−146 . (6.3) Proposition: Let V, W, and Y be vector spaces over a field F and let α : V → W and β : W → Y be linear transformations. Then βα : V → Y is a linear transformation. Proof: If v1 , v2 ∈ V and if a ∈ F then (βα)(v1 + v2 ) = β (α(v1 + v2 )) = β (α(v1 ) + α(v2 )) = β(α(v1 )) + β(α(v2 )) = (βα)(v1 ) + (βα)(v2 ) and (βα)(cv1 ) = β (α(cv1 )) = β(cα(v1 )) = cβ (α(v1 )) = c(βα)(v1 ), which proves the proposition.

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Example: It is often important and insightful to write a linear transformation as a composite of linear transformations of predetermined types. Consider the following situation: let a < b be real numbers and let V be the vector space over R consisting of all functions from the closed interval [a, b] to R. Let W be the subspace of V consisting of all differentiable functions, and let δ : W → V be the function which assigns to each function f ∈ W its derivative. For each real number a < c < b, let εc : V → R be the linear transformation defined by εc : g → g(c). Then the Intermediate Value Theorem from calculus says that the linear transformation β : W → R defined by β : f →

f (b) − f (a) b−a

is of the form εc δ for some c. Let V and W be vector spaces over a field F and let α : V → W be a linear transformation. For w ∈ W, we will denote the set {v ∈ V | α(v) = w} by α−1 (w). Note that this set may be empty. In particular, we will be interested in α−1 (0W ) = {v ∈ V | α(v) = 0W }. This set is called the kernel of α and is denoted by ker(α). Then ker(α) is never empty, since it always contains 0V . If U is a nonempty subset of W, set α−1 (U ) = {α−1 (u) | u ∈ U }. It is easy to verify that α−1 (U ) is a subspace of V whenever U is a subspace of W. Example: Let F be a field and let α ∈ Hom(F 3 , F 4 ) be the linear     a−b a  0   transformation defined by α :  b  →   c  . Then ker(α) = c c     a   a  a∈F .   0 (6.4) Proposition: Let V and W be vector spaces over a field F and let α ∈ Hom(V, W ). Then ker(α) is a subspace of V, which is trivial if and only if α is monic. Proof: Let v1 , v2 ∈ ker(α) and let a ∈ F. Then α(v1 + v2 ) = α(v1 ) + α(v2 ) = 0W + 0W = 0W and so v1 + v2 ∈ ker(α). Similarly, α(av1 ) = aα(v1 ) = a0W = 0W and so av1 ∈ ker(α). This proves that ker(α) is a subspace of V.


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If α is monic then α−1 (w) can have at most one element for each w ∈ W, and so, in particular, ker(α) = {0V }. Conversely, suppose that ker(α) is trivial and that there exist elements v1 = v2 of V satisfying α(v1 ) = α(v2 ). Then α(v1 − v2 ) = α(v1 ) − α(v2 ) = 0W and so v1 − v2 ∈ ker(α). Thus v1 − v2 = 0V and so v1 = v2 , which is a contradiction. Hence α must be monic. Let V and W be vector spaces over a field and let α : V → W be a linear transformation. The image of α is the subset im(α) = {α(v) | v ∈ V } of W. This set is nonempty since 0W = α(0V ) ∈ im(α). Note that w ∈ im(α) if and only if α−1 (w) = ∅. If U is a nonempty subset of V, we denote the subset {α(u) | u ∈ U } of W by α(U ). Thus α(V ) = im(α). (6.5) Proposition: Let V and W be vector spaces over a field F and let α ∈ Hom(V, W ). Then im(α) is a subspace of W, which is improper if and only if α is epic. Proof: If α(v1 ) and α(v2 ) are in im(α) and if a ∈ F, then α(v1 ) + α(v2 ) = α(v1 + v2 ) ∈ im(α) and similarly aα(v1 ) = α(av1 ) ∈ im(α), proving that im(α) is a subspace of W. The second part follows immediately from the definition of an epic function. A monic linear transformation between vector spaces over a field F is called a monomorphism; an epic linear transformation between vector spaces is called an epimorphism. A bijective linear transformation between vector spaces is called an isomorphism. If both spaces are also F -algebras, then a bijective homomorphism of F -algebras is called an isomorphism of F -algebras. Similarly, a bijective homomorphism of unital F -algebras is an isomorphism of unital F -algebras. Example: Let F be a field and let k and n be positive integers. For each matrix A = [aij ] ∈ Mk×n (F ) we can define the transpose of A to be the matrix AT ∈ Mn×k (F ) obtained from A by interchanging its   a11 . . . ak1  ..  . It is easy rows and columns. In other words, AT =  ... .  a1n to check that the function A → A to Mn×k (F ).

T

...

akn

is an isomorphism from Mk×n (F )

Example: Let K and L be F -algebras. It is possible for a linear transformation α : K → L to be an isomorphism of vector spaces without being an isomorphism of F -algebras. This with√ the √ is the case, for example, √ √ linear transformation α : Q( 2) → Q( 5) given by α : a+b 2 → a+b 5.

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Example: Let V be a vector space over a field F. Any linear transformation α : V → F other than the 0-function is an epimorphism. Indeed, if α is a nonzero linear transformation and if v0 ∈ V satisfies the condition that α(v0 ) = c = 0, then for any a ∈ F we have a = (ac−1 )c = (ac−1 )α(v0 ) = α (ac−1 )v0 ∈ im(α). Example: Let Fbe a field and let α : F (∞) → F [X] be the function ∞ defined by α : f → i=0 f (i)X i , which is well-defined since only finitelymany of the f (i) are nonzero. This is easily checked to be an isomorphism of vector spaces. We have already seen that if D is a basis of a vector space V over a field F then there exists a bijective function θ : F (D) → V, and it is easy to verify that this is in fact an isomorphism of vector spaces. This leads us to the very important observation that for any nontrivial vector space V over a field F there exists a nonempty set Ω and an isomorphism F (Ω) → V. Let V and W be vector spaces over a field F and let B be a basis of V. Then we can define a function ϕ : Hom(V, W ) → W B by restriction: ϕ(α) : u → α(u) for all u ∈ B. It is straightforward to check that ϕ is a linear transformation of vector spaces over F. Moreover, by Proposition 6.2 we see that any function f ∈ W B is of the form ϕ(α) for a unique element α of Hom(V, W ). Therefore ϕ is an isomorphism. Let V and W be vector spaces over a field F . If α : V → W is a linear transformation and 0W = w ∈ W then α−1 (w) is not a subspace of V. However, the next result shows that, if it is nonempty, it is “close” to being a subspace. (6.6) Proposition: Let α : V → W be a linear transformation of vector spaces over a field F and let w ∈ im(α). For any v0 ∈ α−1 (w) we have α−1 (w) = {v + v0 | v ∈ ker(α)}. Proof: If v ∈ ker(α) then α(v +v0 ) = α(v)+α(v0 ) = 0W +w = w and so v + v0 ∈ α−1 (w). Conversely, if v1 ∈ α−1 (w) then v1 = (v1 − v0 ) + v0 , where v1 − v0 ∈ ker(α) since α(v1 − v0 ) = α(v1 ) − α(v0 ) = w − w = 0W . Note that α−1 (w) is not a subspace of V but rather the result of “shifting” a subspace by adding a fixed nonzero vector to each of its elements. Such a subset of a vector space is called an affine subset of a vector space. Let V and W be vector spaces over a field F. An affine transformation ζ : V → W is a function of the form v → α(v) + y, for some fixed


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α ∈ Hom(V, W ) and y ∈ W. It is clear that the sum of two affine transformations is again an affine transformation, as is the product of an affine transformation by a scalar, so that the set Af f (V, W ) of all affine transformations from V to W is also a subspace of W V which in turn contains Hom(V, W ) as a subspace. Indeed, Af f (V, W ) = F (Hom(V, W ) ∪ K), where K is the set of all constant functions from V to W. Moreover, if ζ : V → W is the affine transformation defined by v → α(v) + y and if w ∈ W, then ζ −1 (w) = α−1 (w − y) and so is an affine subset of V. Analysis of computational procedures in linear algebra often hinges on the fact that when we think we are computing the effect of some linear transformation α ∈ Hom(V, W ), we are in fact computing that of an affine transformation v → α(v) + y where y is a vector arising from computational or random errors which, hopefully, is “very small” (in some sense) relative to α(v). Similarly, in linear models in statistics one must allow for such an affine transformation, where y is a random error vector, assumed to have expectation 0. Example: Let V = C(0, 1) and let W be the subspace of V composed of all differentiable functions having a continuous derivative. Let δ : W → V be the linear transformation which assigns to each function f ∈ W its derivative. Then ker(δ) consists of all constant functions. If 4x g ∈ im(δ) then g = δ(f ), where f is the function f : x → 0 g(t)dt. 4x Thus δ −1 (g) consists of all functions of the form f : x → 0 g(t)dt + c, where c ∈ R. (6.7) Proposition: If α : V → W is an isomorphism of vector spaces over a field F then there exists an isomorphism β : W → V satisfying βα(v) = v and αβ(w) = w for all v ∈ V and all w ∈ W. Proof: Define the function β by β(w) = v if and only if w = α(v). This function is well-defined since every element w is of the form α(v) for a unique element v ∈ V. It is easy to check that the function β is an isomorphism which satisfies the stated conditions. The function β defined in Proposition 6.7 is denoted by α−1 . Let V and W be vector spaces over a field F. If there exists an isomorphism from V to W we, say that V and W are isomorphic, and write V ∼ = W. It is easy to see that if V, W, and Y are vector spaces over F then: (1) V ∼ =V; (2) If V ∼ = W then W ∼ =V; ∼ (3) If V = W and W ∼ = Y then V ∼ = Y.

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It is also clear that if α : V → W is an isomorphism between vector spaces over F and if B is a basis of V then {α(u) | u ∈ B} is a basis of W. As an immediate consequence of this, we see that if V ∼ = W then the dimensions of V and W are the same. The converse is true if V and W are finitely generated, as we shall now see. (6.8) Proposition: If V and W are vector spaces of finite ∼ W. dimension n over a field F, then V = Proof: Let B = {v1 , . . . , vn } be a basis for V and D = {w1 , . . . , wn } be a basis for W. Define the function f ∈ W B by setting f : vi → wi for all 1 ≤ i ≤ n. By Proposition 6.2, we know that there exists a linear transformation α ∈ Hom(V, W ) satisfying the condition α(vi ) = f (vi ) for all 1 ≤ i ≤ n. This ncontains a n linear transformation is epic since im(α) a v ∈ ker(α) then 0 = α(v) = α ( basis of W. If v = W i=1 ai vi ) = n i=1 i i n a α(v ) = a w and so a = 0 for all 1 ≤ i ≤ n, since the set i i i=1 i i=1 i i D is linearly independent. Therefore ker(α) is trivial, and this shows that α is monic and hence an isomorphism. (6.9) Proposition: If V and W are finitely-generated vector spaces over a field F then (1) There exists a monomorphism from V to W if and only if dim(V ) ≤ dim(W ); (2) There exists an epimorphism from V to W if and only if dim(V ) ≥ dim(W ). Proof: (1) If there exists a monomorphism α from V to W then V ∼ = im(α) and so dim(W ) ≥ dim(im(α)) = dim(V ). Conversely, assume that dim(V ) ≤ dim(W ). Then there exists a basis B = {v1 , . . . , vn } of V and there exists a basis D = {w1 , . . . , wt } of W, where n ≤ t. The function from B to W given by vi → wi for all 1 ≤ i ≤ n can be extended to a linear transformation α : V → W, which is monic and so is a monomorphism. (2) If there exists an epimorphism α from V to W and if {v1 , . . . , vn } is a basis of V, then {α(vi ) | 1 ≤ i ≤ n} is a generating set of W and so the dimension of W is at most n = dim(V ). Conversely, if n = dim(V ) ≥ dim(W ) = t, pick a basis {w1 , . . . , wt } of W and a basis B = {v1 , . . . , vn } of V. Define a function f : B → W by

wi for 1 ≤ i ≤ t . f : vi → wt for t ≤ i ≤ n From Proposition 6.2, it follows that there exists a linear transformation α : V → W satisfying α(vi ) = f (vi ) for all 1 ≤ i ≤ n, and this is the desired epimorphism.


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(6.10) Proposition: Let V and W be vector spaces over a field F, where V is finitely generated. Then dim(V ) = dim(im(α)) + dim(ker(α)) for any linear transformation α ∈ Hom(V, W ). Proof: Let α ∈ Hom(V, W ). Set V1 = ker(α) and let V2 be a complement of V1 in V. By Proposition 5.16, we see that dim(V ) = dim(V1 )+dim(V2 ) and so it suffices for us to show that V2 ∼ = im(α). Let α2 be the restriction of α to V2 . Then α2 ∈ Hom(V2 , im(α)). If v2 ∈ ker(α2 ) then v2 ∈ V2 ∩ V1 = {0V }. Thus α2 is a monomorphism. If w ∈ im(α) then there exists an element v of V satisfying α(v) = w. Moreover, v = v1 +v2 for some v1 ∈ V1 and v2 ∈ V2 so w = α(v) = α(v1 )+α(v2 ) = 0W + α(v2 ) = α(v2 ) = α2 (v2 ). Therefore im(α2 ) = im(α), showing that α2 is also an epimorphism and hence the desired isomorphism. Let V and W be vector spaces over a field F. If α ∈ Hom(V, W ) then we define the rank rk(α) of α to be dim(im(α)) and define is the nullity null(α) of α to be dim(ker(α)). Thus, Proposition 6.10 says that V has finite dimension n then both the rank and nullity of α are finite and their sum is n. The converse is also clearly true: if the rank and nullity of α are both finite, then the dimension of V is finite. Let us give bounds on the rank and nullity of compositions of linear transformations. (6.11) Proposition (Sylvester’s Theorem): Let V, W, and Y be vector spaces finitely-generated over a field F and let α : V → W and β : W → Y be linear transformations. Then (1) null(βα) ≤ null(α) + null(β); (2) rk(α) + rk(β) − dim(W ) ≤ rk(βα) ≤ min{rk(α), rk(β)}. Proof: (1) Let β 1 be the restriction of β to im(α). Then ker(β 1 ) is a subspace of ker(β). By Proposition 6.10, we have null(βα) = dim(V ) − rk(βα) = [dim(V ) − rk(α)] + [rk(α) − rk(βα)] = null(α) + null(β 1 ) ≤ null(α) + null(β). (2) Clearly im(βα) is a subspace of im(β) and so its dimension is no greater than that of im(β). Moreover, im(βα) = im(β 1 ) and so rk(βα) ≤ rk(α). Thus rk(βα) ≤ min{rk(α), rk(β)}. Moreover, from (1) we see that dim(V ) − null(βα) ≥ dim(V ) − null(α) + dim(W ) − null(β) − dim(W ) = rk(α) + rk(β) − dim(W ) and this proves that rk(α) + rk(β) − dim(W ) ≤ rk(βα).

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Exercises Exercise 197 Which of the following statements are true for all vector spaces V and W over a field F and all α ∈ Hom(V, W )? (1) α(A ∪ B) = α(A) ∪ α(B) for all nonempty subsets A and B of V ; (2) α(A ∩ B) = α(A) ∩ α(B) for all nonempty subsets A and B of V ; (3) α−1 (C ∪ D) = α−1 (C) ∪ α−1 (D) for all nonempty subsets C and D of W ; (4) α−1 (C ∩ D) = α−1 (C) ∩ α−1 (D) for all nonempty subsets C and D of W. Exercise 198 Let α : R3 → R3 be a linear transformation satisfying         1 −1 1 0 α  0  =  3  , α  −1  =  1  , 1 4 1 0       1 3 1 and α  2  =  1  . What is α  0 ? −1 4 0 Exercise 199 Let α : R3 → R3 be a linear transformation satisfying           1 1 1 0 0 α  1  =  2  , α  0  =  1  , and α  −1  = 0 −1 −1 1 1     1 3  3  . Find a vector v ∈ R3 for which α(v) =  0  . 0 3 Exercise 200 Let F be a field and let V be the subspace of F [X] consisting of all polynomials of degree at most 2. Let α : V → F [X] be a linear transformation satisfying α(1) = X, α(X + 1) = X 5 + X 3 , and α(X 2 + X + 1) = X 4 − X 2 + 1. What is α(X 2 − X)? Exercise 201 For each d ∈ R, let αd : R2 → R2 be the function defined ! ! a a + b + d2 + 1 by αd : → . Is there a number d having the b a property that αd is a linear transformation? Exercise 202 For each d ∈ R, let αd : R2 → R2 be the function defined ! ! a 5da − db . Is there a number d having the by αd : → b 8d2 − 8d − 6 property that αd is a linear transformation?


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Exercise 203 Let W and W be subspaces of a vector space V over a field F and assume that we have linear transformations α : W → V and β : W → V satisfying the condition that α(v) = β(v) for all v ∈ W ∩W . Find a linear transformation θ : W + W → V, the restriction of which to W equals α and the restriction of which to W equals β, or show why no such linear transformation exists. Exercise 204 Let F = GF (3) and let θ ∈ F F be the function defined by θ(0) = 0, θ(1) = 2, and θ(2) = 1. Let n be a positive integer and     a1 θ(a1 )     .. let α : F n → F n be the function defined by α :  ...  →   Is . an

θ(an )

α a linear transformation? Exercise 205 Does there exist a linear transformation α : Q4 → Q[X]       1 −1 −1  2   1   4        satisfying α   0  = 2, α  1  = X, and α  2  = −1 1 1 X + 1? Exercise 206 Let B be a Hamel basis for R as a vector space over Q and let 1 = a ∈ R. Show that there exists an element y ∈ B satisfying ay ∈ / B. Exercise 207 For which nonnegative  integers   a GF (3)3 to itself defined by α :  b  →  c tion?

h  is the function α from ah b  a linear transformach

Exercise 208 For any field F, let θ : F → F be the function defined by

0 if a = 0 . θ : a → a−1 otherwise This is clearly a linear transformation when F = GF (2). Does there exist a field other than GF (2) for which θ is a linear transformation? Exercise 209 Let V = F ∞ and let α : V → V be the function that assigns to each sequence 2 , . . .] ∈ V +its sequence of partial sums, namely * [a1 , a 2 3 [a1 , a2 , . . .] → a1 , i=1 ai , i=1 ai , . . . . Is α a linear transformation? Exercise 210 Let Y = RR × R. Is the function α : Y → R defined by α : (f, a) → f (a) a linear transformation?

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Exercise 211 Let α : R → R be a continuous function satisfying α(a + b) = α(a) + α(b) for all a, b ∈ R. Show that α is a linear transformation. Exercise 212 Let F be a field and let b and c be nonzero elements of F. Let α : F ∞ → F ∞ be the linear transformation defined by α : [a1 , a2 , . . .] → [a3 + ba2 + ca1 , a4 + ba3 + ca2 , . . .]. Let y ∈ ker(α) be a vector satisfying the condition that two successive entries in y equal 0. Show that y = [0, 0, . . .]. √ Exercise 213 Consider the field F = Q( 2) as a Q-algebra. Show that the only homomorphisms of Q-algebras from√ F to itself are the identity √ function and the function a + b 2 → a − b 2. Exercise 214 Let V, W, and Y be vector spaces finitely-generated over a field F and let α : V → W be a linear transformation. Show that the set of all linear transformations β : W → Y satisfying the condition that βα is the 0-transformation is a subspace of Hom(W, Y ), and calculate its dimension. Exercise 215 Let V and W be vector spaces over a field F and let V be a proper subspace of V. Are {α ∈ Hom(V, W ) | ker(α) ⊆ V } and {α ∈ Hom(V, W ) | ker(α) ⊇ V } subspaces of Hom(V, W )? Exercise 216 Let V and W be vector spaces over a field F and assume that there are subspaces V1 and V2 of V, both of positive dimension, satisfying V = V1 ⊕ V2 . For i = 1, 2, let Ui = {α ∈ Hom(V, W ) | ker(α) ⊇ Vi }. Show that {U1 , U2 } is an independent set of subspaces of Hom(V, W ). Is it necessarily true that Hom(V, W ) = U1 ⊕ U2 ? Exercise 217 Let F be a field, and let α : M2×2 (F ) → M2×2 (F ) be a linear transformation satisfying α(AB) = α(A)α(B) for all A, B ∈ ! 0 0 I. = M2×2 (F ). Show that α 1 0 Exercise 218 Let V and W be vector spaces over a field F and let α, β : V → W be linear transformations satisfying the condition that for each v ∈ V there exists a scalar cv ∈ F (depending on v) satisfying β(v) = cv α(v). Show that there exists a scalar c satisfying β = cα. Exercise 219 Find the kernel of the linear transformation α : R5 → R3   a    b  b + c − 2d + e      defined by α :   c  → a + 2b + 3c − 4d .  d  2a + 2c − 2e e


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Exercise 220 Let α : R3 → R3 be the linear transformation defined by     a 2a + 4b − c  . Are im(α) and ker(α) disjoint? 0 α :  b  →  c 3c + 2b − a       2 1 1       0   1  −1        Exercise 221 Let W be the subspace Q  , , of 0   0   0       1 1 1 Q4 and let α : W → Q2 be the linear transformation defined by setting   a !  b  a + 2b + c   α: → . Find a basis for ker(α). c  −a − 2b − c d Exercise 222 Let F = GF (3) and let α : F 3 → F 3 be the linear     a a+b transformation defined by α :  b  →  2b + c  . Find the kernel of c 0 α. Exercise 223 Let α : R4 → R3 be the linear transformation defined by     a 2a + 4b + c − d  b    3a + b − 2c  . Do there exist a, b, d ∈ Z such that α:  c  → a + 5c + 4d d   a  b     7  ∈ ker(α)? d Exercise 224 Let V and W be vector spaces over a field F. Let α ∈ Hom(V, W ) and β ∈ Hom(W, V ) satisfy the condition that αβα = α. If w ∈ im(α), show that α−1 (w) = {β(w) + v − βα(v) | v ∈ V }. Exercise 225 Let V, W, and Y be vector spaces over a field F and let α ∈ Hom(V, W ) and β ∈ Hom(W, Y ) satisfy the condition that im(α) has a finitely-generated complement in W and im(β) has a finitely-generated complement in Y. Does im(βα) necessarily have a finitely-generated complement in Y ? Exercise 226 Let α : M3×3 (R) → R be the function defined by α : 3 3 [aij ] → i=1 j=1 aij . Show that α is a linear transformation and find a basis for ker(α).

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Exercise 227 Let F = GF (2) and let n > 2 be an integer. Let W be   a1   the set of all vectors  ...  in F n having an even number of nonzero an entries. Show that W is a subspace of F n by showing that it is the kernel of some linear transformation. Exercise 228 Let A and B be nonempty sets. Let V be the collection of all subsets of A and let W be the collection of all subsets of B, both of which, as we have seen, are vector spaces over GF (2). Any function f : A → B defines a function αf : W → V by setting αf : D → {a ∈ A | f (a) ∈ D}. Show that each such function αf is a linear transformation, and find its kernel. Exercise 229 Let V be a vector space over a field F and let α : V 3 → V   v1 be the function defined by α :  v2  → v1 + v2 + v3 . Show that α is a v3 linear transformation and find its kernel. Exercise 230 Let n be a positive integer and let V be the subspace of R[X] composed of all polynomials of degree at most n. Let α : V → V be the linear transformation given by α : p(X) → p(X + 1) − p(X). Find ker(α) and im(α). Exercise 231 Let α : R3 → R3 be the linear transformation given by     a a+b+c α :  b  →  −a − c  . Find ker(α) and im(α). c b Exercise 232 Find the kernel of the linear transformation α : Q[X] → R √ defined by α : p(X) → p( 3). Exercise 233 Let V = C(0, 1). For each positive integer n, we define the nth Bernstein function β n : V → R[X] by β n : f →

n k=0

n! f k!(n − k)!

k X k (1 − X)n−k . n

∞ Show that each β n is a linear transformation and find n=1 ker(β n ). (Note: the Bernstein functions are used in building polynomial approximations to continuous functions.)


95

Exercise 234 Let V and W be vector spaces over a field F, where dim(V ) is a positive integer. Show that W = {im(α) | α ∈ Hom(V, W )}. Exercise 235 Let W be the subspace of RR consisting of all twicedifferentiable functions and let α : W → RR be the linear transformation α : f → f . Find α−1 (f0 ), where f0 ∈ RR is defined by f0 : x → x + 1. Exercise 236 Let W be the subspace of RR consisting of all differbe the function defined by entiable functions and let α : W → RR α(f ) : x → f (x) + cos(x)f (x). Show that α is a linear transformation and find its kernel. Exercise 237 Let n be a positive integer and let V be a vector space over C. Does there exist a linear transformation α : V → Cn other than the 0-function satisfying the condition that im(α) ⊆ Rn ? Exercise 238 Let V and W be vector spaces over a field F and let α : V → W be a linear transformation other than the 0-function. Find a linear transformation β : V → W satisfying im(α) = im(β) = im(α + β). Exercise 239 Let V be a finite-dimensional vector space over a field F and let α, β ∈ Hom(V, V ) be linear transformations satisfying im(α) + im(β) = V = ker(α) + ker(β). Show that im(α) ∩ im(β) = {0V } = ker(α) ∩ ker(β). Exercise 240 Let V, W, and Y be vector spaces over a field F and let α ∈ Hom(V, W ) and β ∈ Hom(W, Y ) satisfy the condition that ker(α) and ker(β) are both finitely generated. Is ker(βα) necessarily finitely generated? Exercise 241 Find a linear transformation α : Q3 → Q4 satisfying  1    2   2     1  −1      im(α) = Q  , . 3   1       −4 0 Exercise Let F = GF (2) and let α ∈ Hom(F 7 , F 3 ) be given by  242    a1 a4 + a5 + a6 + a7  ..   .  →  a2 + a3 + a6 + a7  . If v is a nonzero element of ker(α), a1 + a3 + a5 + a7 a7 show that at least three entries in v are equal to 1. Exercise 243 Let V and W vector spaces finite dimensional over a field F and let α ∈ Hom(V, W ). If Y is a subspace of W, is it true that dim(α−1 (Y )) ≥ dim(V ) − dim(W ) + dim(Y )?

96


Exercise 244 Let V be a vector space over a field F and let Y = V ∞ . Let W be the subspace of Y consisting of all those sequences [v1 , v2 , . . .] in which vi = 0 for all odd i and let W be the subspace of Y consisting of all those sequences in which vi = 0 for all even i. Find a linear transformation from Y to itself, the kernel of which equals W and the image of which equals W . Exercise 245 Let W be the subspace of R6 composed of all vectors   a1 6  ..   .  satisfying i=1 ai = 0. Does there exist a monomorphism from a6 W to R4 ? Exercise 246 Let n be a positive integer and let α : Qn → Qn be a linear transformation which is not a monomorphism. Does there necessarily exist a nonzero element of ker(α) all the entries of which are integers? Exercise 247 Let n be a positive integer and let W be the subspace of C[X] consisting of all polynomials of degree less than n. Let a1 , . . . , an be distinct complex numbers and let α : W → Cn be the function defined by   p(a1 )   .. α : p(X) →   . Is α a monomorphism? Is it an isomorphism? . p(an ) Exercise 248 Let V be a vector space over a field F and let α : V → V be a linear transformation satisfying the condition that α2 = aα + bσ 1 , where a and b are nonzero scalars. Show that α is a monomorphism. Exercise 249 Let p be a prime integer and let F be a field of characteristic p. Let (K, •) be an associative and commutative unital F -algebra and let α : K → K be the function defined by α : v → v p . Show that α is an isomorphism of unital F -algebras. Exercise 250 Let F be a field and let K and K be fields containing F. Show that every homomorphism of F -algebras K → K is a homomorphism of unital F -algebras. Exercise 251 Let F = GF (7). How many distinct monomorphisms can one define from F 2 to F 4 ? Exercise 252 Let V and W be vector spaces over a field F and let α, β ∈ Hom(V, W ) be monomorphisms. Is α + β necessarily a monomorphism? Exercise 253 Let F be a field and let F be a field containing F. Let (K, •) be an F -algebra and let α : F → K be a nontrivial homomorphism of F -algebras. Show that α is monic.


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Exercise 254 Let V and W be vector spaces over a field F and let α ∈ Hom(V, W ) be an epimorphism. Show that there exists a linear transformation β ∈ Hom(W, V ) satisfying the condition that αβ is the identity function on W. Exercise 255 Let V be a vector space finite dimensional over a field F , the dimension n of which is even. Show that there exists an isomorphism α : V → V satisfying the condition that α2 (v) = −v for all v ∈ V. Exercise 256 Let α : V → W be a linear transformation between vector spaces over a field F and let D be a nonempty linearly-independent subset of im(α). Show that there exists a basis B of V satisfying the condition that {α(v) | v ∈ B} = D. Exercise 257 Let V and W be vector spaces over a field F and let α ∈ Hom(V, W ) satisfy the condition that αβα is not the 0-function for any linear transformation β : W → V which is not the 0-function. Show that α is an isomorphism. Exercise 258 Let F be a field and let α : F 3 → F [X] be the linear   a transformation defined by  b  → (a + b)X + (a + c)X 5 . Find the nullity c and rank of α. Exercise 259 Let F be a field and let p(X) = X 2 + bX + c ∈ F [X] be a polynomial having distinct nonzero roots d1 and d2 in F. Let α : F 3 → F be the linear transformation defined by   a1  a2  → a3 + ba2 + ca1 a3 and let β : F ∞ → F ∞ be the linear transformation defined by β : [a1 , a2 , a3 , . . .] → [α(a1 , a2 , a3 ), α(a2 , a3 , a4 ), . . .] . Show that the nullity of β is at least 2. Exercise 260 Let Ω be a nonzero set and let V be the collection of all subsets of Ω, considered as a vector space over GF (2). Show that this vector space is isomorphic to GF (2)Ω . Exercise 261 Let F be a field and let V be the subspace of F ∞ consisting of all sequences [a1 , a2 , a3 , . . .] in which ai = 0 for all even i. Let W be the subspace of F ∞ consisting of all sequences [a1 , a2 , a3 , . . .] in which ai = 0 for all odd i. Show that V ∼ = W. = F∞ ∼

98


Exercise 262 Let V be a vector space over a field F having subspaces !

w W and W . Let Y = w ∈ W and w ∈ W , which is w a subspace of V 2 . Let α : Y → V be the linear transformation defined ! w → w + w . Find the kernel of α, and show that it is by α : w isomorphic to W ∩ W . Exercise 263 Let V be a vector space over a field F. Let W be a subspace of V and let W be a complement of W in V. Let α : W → W be a linear transformation. Show that W isomorphic to the subspace Y = {w + α(w) | w ∈ W } of V. Exercise 264 Show that there is no vector space over any field F having precisely 15 elements. Exercise 265 Let F be a field and let V = F [X]. Show that V ∼ = V 2. Exercise 266 Let V, W, and Y be vector spaces over a field F . Let {α1 , . . . , αn } be a finite subset of Hom(V, W ) and let β ∈ Hom(V, Y ) 5n be a linear transformation satisfying ker(αi ) ⊆ ker(β). Show that i=1 thereexist linear transformations γ 1 , . . . , γ n in Hom(W, Y ) satisfying n β = i=1 γ i αi . Exercise 267 Let V be a vector space over a field F and let W be a subspace of V. For each v ∈ V, let v + W = {v + w | w ∈ W }. Let V /W be the collection of all the sets of the form v + W for v ∈ V and define operations of addition and scalar multiplication on V /W by setting (v + W ) + (v + W ) = (v + v ) + W and c(v + W ) = (cv) + W for all v, v ∈ V and c ∈ F. Show that: (1) v + W = v + W if and only if v − v ∈ W ; (2) V /W, with the given operations, is a vector space over F ; (3) The function v → v + W is an epimorphism from V to W, the kernel of which equals W ; (4) Every complement of W in V is isomorphic to V /W. The space V /W is called the factor space of V by W. Exercise 268 Let F be a field and let m > n be positive integers. Let A and B be fixed matrices in Mn×m (F ) and let θ : Mn×m (F ) → Mn×m (F ) be the linear transformation defined by θ : C → ACB. Show that θ is not an isomorphism.

7 The endomorphism algebra of a vector space

Let V be a vector space over a field F. A linear transformation α from V to itself is called an endomorphism of V. We will denote the set of all endomorphisms of V by End(V ). This set is nonempty, since it includes the functions of the form σ c : v → cv for c ∈ F. In particular, it includes the 0-endomorphism σ 0 : v → 0V and the identity endomorphism σ 1 : v → v. If V is nontrivial, these functions are not the same. We see that we have two operations defined on End(V ) : addition and multiplication (given by composition). Indeed, as a direct consequence of the definitions we conclude the following: (7.1) Proposition: If V is a nontrivial vector space over a field F, then End(V ) is an associative unital F -algebra with σ 0 being the identity element for addition and σ 1 being the identity element for multiplication. If V is a nontrivial vector space over a field F then there exists a function σ : F → End(V ) defined by σ : c → σ c for all c ∈ F. This function is monic, for if σ c = σ d then for any 0V = v ∈ V we have cv = σ c (v) = σ d (v) = dv and hence (c − d)v = 0V . Since 0V = v, this implies that c − d = 0 and so c = d. Moreover, if c, d ∈ F then σ c + σ d = σ c+d and σ c σ d = σ cd so σ is a monic homomorphism of unital F -algebras. We can use this function to identify F with its image under σ and consider it a subalgebra of the F -algebra End(V ). 99

100

7. The endomorphism algebra of a vector space

If α, β ∈ End(V ) and if c ∈ F, then we have already seen that the functions α + β, αβ, ). Therefore we n and cα all belong to End(V n see that if p(X) = i=0 ai X i ∈ F [X] then p(α) = i=0 ai αi is an endomorphism of V, and, indeed, the set F [α] of all endomorphisms of V of this form is an F -subalgebra of End(V ). The function from F [X] to F [α] given by p(X) → p(α) is immediately seen to be an epic homomorphism of unital F -algebras for any α ∈ End(V ). Example: Let F = GF (2) and let p(X) = X 2 + X ∈ F [X]. Then p(a) = 0 for every !a ∈ F. However, p(α) = σ 0 , where α ∈ End(F 2 ) is ! a b defined by α : → . b a Example: Structures of the form F [α] are important in many areas of mathematics. For example, let V be the collection of all infinitelydifferentiable functions from R to R and let δ be the differentiation n i endomorphism on V . If p(X) = i=0 ai X ∈ R[X], then we have n [i] [i] denotes the ith derivative of f . p(δ) : f → a0 f + i=1 ai f , where f Such an endomorphism is called a differential operator with constant coefficients on V. If c ∈ R and if f ∈ V is the function by n given cx i cx : x → e , then δ(f ) = cf and so p(δ) : f → a c e = f c c c c i=0 i n i f a c = p(c)f . Thus, p(δ) is the 0-function whenever c is as c c i=0 i root of p(X). Hence fc ∈ ker(p(δ)) for each root c of p(X). Example: Let F be a field and let (K, •) be a nonassociative F algebra. An endomorphism δ ∈ End(K) is a derivation if and only if δ(v • w) = [δ(v)] • w + v • [δ(w)] . Thus, for example, if K is a Lie algebra then, as a consequence of the Jacobi identity, we see that every y ∈ K defines a derivation δ y of K given by δ y : v → y • v. Also, if K is the R-algebra consisting of all infinitely-differentiable functions in RR , then the endomorphism of K which assigns to each function in K its derivative is a derivation. The set of all derivations defined on K is a subspace of End(K). If δ and δ are derivations on K, then δδ is not, in general, a derivation on K, but the Lie product δδ − δ δ is always a derivation on K, and so the set of all derivations on K is a Lie algebra over F. Given a nontrivial vector space V over a field F, we note that the F algebra End(V ) is neither necessarily commutative nor necessarily entire, as the following examples show: Example: Let F be a field and let V = F 3 . Let α, β ∈ End(V ) be       a b a the endomorphisms defined by α :  b  →  a  and β :  b  → c c c


101



         a a b a 0  0  . Then βα :  b  →  0  and αβ :  b  →  a  , so 0 c 0 c 0 βα = αβ. 3 Example: Let F be a field andlet  V =F  ) be  . Let  α, β ∈ End(V a 0 a  0  and β :  b  → the endomorphisms defined by α :  b  → c c c   a  0  . Then βα = σ 0 = αβ. 0

We do, however, have the following: (7.2) Proposition: Let V be a nontrivial vector space over a field F. Then for all α ∈ End(V ) and all c ∈ F we have ασ c = σ c α. Proof: If v ∈ V then ασ c (v) = α(cv) = cα(v) = σ c α(v).

An endomorphism of a vector space V over a field F which is also an isomorphism (i.e., which is both monic and epic), is called an automorphism of V. Since α(0V ) = 0V for any endomorphism α of V, we see that any automorphism of V induces a permutation of V {0V }. Similarly, a homomorphism of F -algebras which is also an isomorphism is an automorphism of F -algebras. By what we have already seen, we know that α ∈ End(V ) is an automorphism if and only if there exists an endomorphism α−1 ∈ End(V ) satisfying αα−1 = σ 1 = α−1 α. We will denote the set of all automorphisms of V by Aut(V ). This set is nonempty, since σ 1 ∈ Aut(V ), = σ 1 . Moreover, if α, β ∈ Aut(V ) then (αβ)(β −1 α−1 ) = where σ −1 1 −1 −1 = αα−1 = σ 1 and similarly (β −1 α−1 )(αβ) = σ 1 . Thus α(ββ )α αβ ∈ Aut(V ), with (αβ)−1 = β −1 α−1 . It is also clear that if α ∈ Aut(V ) then α−1 ∈ Aut(V ). Example: Let V be a vector space over a field F and let n > 1 be an integer. Any permutation π of the set {1, . . . , n} defines an     v1 vπ(1)  v2   vπ(2)      automorphism απ of V n given by απ :  .  →  .  which  ..   ..  vn

vπ(n)

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rearranges the entries of each vector according to the permutation π. More generally, if V is a vector space over a field F having a basis B = {vi | i ∈ Ω} and if π isa permutation of Ω, then there is an automorphism a v → of V defined by i i i∈Λ i∈Λ aπ(i) vπ(i) for each finite subset Λ of Ω. Example: Let F be a field and let n be a positive integer. We have already seen that the function A → AT is an automorphism of Mn×n (F ), considered as a vector space over F. Example: Let V be a vector space having finite dimension n over a field F and let v and y be nonzero elements of V. Then there exist satisfying v1 = v and y1 = y. bases {v1 , . . . , vn } and {y1 , . . . , yn } of V n n The function α : V → V defined by α : i=1 ai vi → i=1 ai yi is thus an automorphism of V satisfying α(v) = y. Let V be a vector space over a field F and let n be a positive integer. We will list several types automorphisms, called elementary automorphisms, of a vector space of the form V n . These automorphisms will play an important part in our ensuing discussion.     v1 w1     (1) If 1 ≤ h = k ≤ n, we define εhk ∈ Aut(V n ) by  ...  →  ...  , vn   vk vh wi =  vi

where

wn

if i = h if i = k . otherwise

This automorphism satisfyies ε−1 hk = εhk . (2) If 1 ≤ h ≤ n, and if 0 = c ∈ F, we define εh;c ∈ Aut(V n ) by     v1 w1  ..   ..   .  →  .  , where vn

wn

wi =

cvi vi

if i = h . otherwise

This automorphism satisfyies ε−1 h;c = εh,c−1 . (3) If 1 ≤ h = k ≤ n and if c ∈ F, we define εhk;c ∈ Aut(V n ) by     v1 w1  ..   .   .  →  ..  , where vn

wn

wi =

vi + cvk vi

if i = h . otherwise


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This automorphism satisfyies ε−1 hk;c = εhk;−c . Identifying the automorphisms of a finite-dimensional vector space V over a field F is a problem which will be of major importance to us later, and so it is important to characterize these functions. (7.3) Proposition: Let V be a vector space of finite dimension n over a field F . Then the following conditions on an endomorphism α of V are equivalent: (1) α is an automorphism of V ; (2) α is monic; (3) α is epic. Proof: By definition, (1) implies (2). Now assume (2). By Proposition 6.10, we see that the rank of α equals n and so im(α) = V by Proposition 5.11, proving (3). Now assume (3). By Proposition 6.10, we see that the nullity of α equals n − n = 0 and so ker(α) = {0V }, proving that α is monic as well, and so is bijective. This proves (1). (7.4) Proposition: Let V be a finite-dimensional vector space over a field F and let α ∈ End(V ). If there exists a β ∈ End(V ) satisfying αβ = σ 1 or βα = σ 1 , then α ∈ Aut(V ) and β = α−1 . Proof: If βα = σ 1 then ker(α) ⊆ ker(σ 1 ) = {0V } and so, by Proposition 7.3, α ∈ Aut(V ). Similarly, if αβ = σ 1 then im(α) ⊇ im(σ 1 ) = V and so, by Proposition 7.3, α ∈ Aut(V ). Moreover, if αβ = σ 1 we see that α−1 = α−1 σ 1 = α−1 (αβ) = β and similarly α−1 = β when βα = σ 1 . Example: Proposition 7.3 and Proposition 7.4 are no longer true if we remove the condition of finite dimensionality. For example, let F be a field and let V = F [X]. α and β of V by setting nDefine the endomorphisms n n n α : i=0 ai X i → i=0 ai X i+1 and β : i=0 ai X i → i=1 ai X i−1 . Then α,β ∈ / Aut(V ), despite the fact that α is monic and β is epic. Moreover, βα = σ 1 but αβ = σ 1 . Let V be a vector space over a field F and let α ∈ End(V ). A subspace W of V is invariant under α if and only if α(w) ∈ W for all w ∈ W or, in other words, if and only if α(W ) ⊆ W. Thus, W is invariant under α if and only if the restriction of α to W is an endomorphism of W. It is clear that V and {0V } are both invariant under every endomorphism of V. If α ∈ End(V ) then im(α) and ker(α) are both invariant under α.

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Example: Let F be a field and, for each positive integer k, let Wk be the subspace of F [X] composed of all polynomials of degree at most k. Let δ be the formal differentiation endomorphism of F [X], namely n n the endomorphism defined by δ : i=0 ai X i → i=0 iai X i−1 . Then each under δ. Now assume that F is of of the subspaces Wk is invariant n characteristic 0. If p(X) = i=0 ai X*i ∈ Wk and + if a ∈ F then it is easy n 1 h to check that p(X) = p(a) + h=1 h! δ (p)(a) (X − a)h . The coefficients * + h 1 are known as the Taylor coefficients of p(X) around a. h! δ (p)(a)

Example: Let V = R2 and let α be the endomorphism of V defined ! ! a b by α : → . Let W be a proper subspace of V which b −a is invariant under α. Then dim(W ) ≤ 1 and so there exists a vector ! ! c d w= satisfying W = Rw. Since α(w) = , it follows that d −c there exists a real number e such that α(w) = ew. That is to say, ec = d and ed = −c. From this we learn that ce2 = −c and so c = d = 0.

!0 This proves that W = , and so we see that V has no proper 0 nontrivial subspaces invariant under α.

Example: Let F

be a field and let n be a positive integer. Let     a1 an  a2   a1      α be the endomorphism of F n defined by α :  .  →  .  .  ..   ..  an an−1 A subspace W invariant under α is cyclic. Cyclic subspaces of F n , where F is a finite field, are important in defining certain families of error-correcting codes.

Let V be a vector space over a field F. An endomorphism α of V is a projection if and only if α2 = α. Note that if α is a projection and if w = α(v) ∈ im(α) then α(w) = α2 (v) = α(v) = w, so that the restriction of α to its image is just σ 1 . The converse is also true. If α ∈ End(V ) satisfies the condition that the restriction of α to its image is just σ 1 , then for each v ∈ V we have α2 (v) = α(α(v)) = σ 1 (α(v)) = α(v) and so α is a projection.


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Example: If F is a field then the endomorphism of F 3 defined by    a 3a − 2c  b  →  −a + b + c  is a projection. c 3a − 2c 

Example: The sum of two projections need example, if V = R3 then the endomorphisms        a a a by α :  b  →  b  and β :  b  →  c 0 c

not be a projection. For α and β of V defined  0 b  are projections, but c

α + β is not a projection. Example: If W is a subspace of a vector space V over a field F having a complement Y in V, we know that every element v ∈ V can be written in a unique way in the form w + y, where w ∈ W and y ∈ Y. The endomorphism of V defined by v → w is a projection the image of which is W. In fact, all projections of a vector space are of the form in the previous example, as the following example shows. (7.5) Proposition: Let V be a vector space over a field F and let α ∈ End(V ) be a projection. Then V = im(α) ⊕ ker(α). Proof: If v ∈ im(α) ∩ ker(α) then there exists an element y of V satisfying v = α(y) and so v = α(v) = 0V . Thus im(α) and ker(α) are disjoint. If v is an arbitrary vector in V then v = [v − α(v)] + α(v) ∈ ker(α) + im(α). Therefore V = im(α) ⊕ ker(α). (7.6) Proposition: Let V be a vector space over a field F and let α ∈ End(V ). A subspace W of V is invariant under α if and only if βαβ = αβ for each projection β of V the image of which is W. Proof: Assume that W is invariant under α and let β be a projection of V the image of which is W. By Proposition 7.5 we have V = W ⊕ker(β). If v ∈ V we can therefore write v = w+y, where w ∈ W and y ∈ ker(β). Hence αβ(v) = αβ(w) + αβ(y) = α(w) + 0V = α(w) = βα(w) = βαβ(v), showing that βαβ = αβ. Conversely, if βαβ = αβ for each projection β of V the image of which is W then, for each such β, we have w = β(w) for all w ∈ W and so α(w) = αβ(w) = βαβ(w) ∈ W, showing that W is invariant under α.

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(7.7) Proposition: Let V be a vector space over a field F and let {W1 , . . . Wn } be a set of subspaces of V. Then the following conditions are equivalent: (1) V = W1 ⊕ . . . ⊕ Wn ; (2) There exist projections α1 , . . . αn in End(V ) with Wi = im(αi ) for all 1 ≤ i ≤ n, which satisfy the conditions αi αj = σ 0 for i = j and α1 + . . . + αn = σ 1 . Proof: (1) ⇒ (2): From n (1) it follows that every v ∈ V can be written in a unique manner as i=1 wi , where wi ∈ Wi for all 1 ≤ i ≤ n. Define αi to be the projection v → wi for each i. It is easy to verify that these linear transformations do indeed satisfy the required conditions. n ⇒ (1): Since α1 +. . .+α n = σ 1 we surely have V = i=1 im(αi ) = (2) n W . If 0 = v ∈ W ∩ W then there exists an i = h such that i V h j i=1 j=h αi (v) = 0V . Butαh (v) = v so αi αh = σ 0 , which is a contradiction. Therefore Wh ∩ j=h Wj = {0V } for each 1 ≤ h ≤ n, proving (1). (7.8) Proposition: Any two complements of a subspace W of a vector space V over a field F are isomorphic.

Proof: Let U and Y be complements of W in V. By Proposition 7.7 we know that there exists a projection β ∈ End(V ) the image of which is U and the kernel of which is W. Let α be the restriction of β to Y. The linear transformation α is a monomorphism since ker(α) ⊆ ker(β) ∩ Y = W ∩ Y = {0V }. Any vector u ∈ U can be written as w + y, where w ∈ W and y ∈ Y and we have α(y) = β(y) = β(w) + β(y) = β(w + y) = β(u) = u. Thus we see that α is also epic and hence is the desired isomorphism. We now introduce a notion which is basic in all branches of mathematics. A relation ≡ defined between the elements of a given nonempty set U is called an equivalence relation if and only if the following conditions are satisfied: (1) u ≡ u for all u ∈ U ; (2) u ≡ u if and only if u ≡ u; (3) If u ≡ u and u ≡ u then u ≡ u . Example: Let B be a nonempty subset of a set A and define a relation ≡B on A by setting a ≡B a if and only if a = a or both a and a belong to B. Then ≡B is an equivalence relation on A. In particular, if W is a subspace of a vector space V then the relation ≡W defined on V by setting v ≡W v if and only if v − v ∈ W is an equivalence relation on V.


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Example: Let V and W be a vector spaces over a field F and let α ∈ HomF (V, W ). Define a relation ≡ on V by setting v ≡ v if and only if α(v) = α(v ). This is easily seen to be an equivalence relation. Let V be a vector space over a field F. A subset G of Aut(V ) is a group of automorphisms if it is closed under taking products, contains σ 1 , and satisfies the condition that α−1 ∈ G whenever α ∈ G. Clearly Aut(V ) itself is such a group. The notion of a group of automorphisms is very important in linear algebra and its applications, but here we will only touch on it. Example: Let V be a vector space over a field F and let Ω be a nonempty set. Every permutation π of Ω defines an automorphism απ of the vector space V Ω over F defined by απ (f ) : i → f (π(i)) for all i ∈ Ω and all f ∈ V Ω . The collection G of all such automorphisms is a group of automorphisms in Aut(V Ω ). (7.9) Proposition: If V is a vector space over a field F and if G is a group of automorphisms of V then G defines an equivalence relation ∼G on V by setting v ∼G v if and only if there exists an element α of G satisfying α(v) = v . Proof: If v ∈ V then σ 1 (v) = v and so v ∼G v. If v, v ∈ V satisfy v ∼G v then there exists an element α of G satisfying α(v) = v and so v = α−1 (v). Thus v ∼G v. Finally, if v, v , v ∈ V satisfy v ∼G v and v ∼G v then there exist elements α and β of G satisfying α(v) = v and β(v ) = v and so βα(v) = v . Thus v ∼G v . (7.10) Proposition: If V is a vector space over a field F and if G is a group of automorphisms of V then all elements of G have the same rank. Proof: If α ∈ G then, by Proposition 6.11, rk(σ 1 ) = rk(αα−1 ) ≤ rk(α) = rk(ασ 1 ) ≤ rk(σ 1 ) and so rk(α) = rk(σ 1 ).

Exercises Exercise 269 Let V be a vector space over GF (3). Show that there exists an endomorphism α of V satisfying α(v) + α(v) = v for all v ∈ V.

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Exercise 270 Let V be a vector space finitely generated over a field F and let α, β, γ ∈ End(V ). Find necessary and sufficient conditions for there to exist an endomorphism θ of V satisfying αγβ = βθα. Exercise 271 Let F = GF (2) and let n be a positive integer. Let     a1 a1  ..   ..  n n α : F → F be the function defined by α :  .  →  .  , where an

an

0 = 1 and 1 = 0. Is α an endomorphism of F n ? Exercise 272 Let α, β : Q[X] → Q[X] be defined by α : p(X) → Xp(X) and β : p(X) → X 2 p(X). Show that α, β, and α − β are all monic endomorphisms of Q[X]. Exercise 273 Let V be a finitely-generated vector space over a field F and let α ∈ End(V ). Show that α is not monic if and only if there exists an endomorphism β = σ 0 of V satisfying αβ = σ 0 . Exercise 274 Let V be a vector space over a field F and let α ∈ End(V ). Show that ker(α) = ker(α2 ) if and only if ker(α) and im(α) are disjoint. Exercise 275 Let V be a vector space over a field F and let α ∈ End(V ). Show that im(α) = im(α2 ) if and only if V = ker(α) + im(α). Exercise 276 Let V be a vector space over a field F and let K = F × V × End(V ), which is again a vector space over F. Define an operation on K by setting (a, v, α) (b, w, β) = (ab, aw + β(v), βα). Is (K, ) an F -algebra? Is it associative? Is it unital? Exercise 277 Let V be a vector space over a field F, and let Af f (V, V ) be the set of all affine transformations from V to itself. Is Af f (V, V ), on which we have defined the operations of addition and composition of functions, an associative unital F -algebra? ! ! a −b → . Exercise 278 Let α ∈ Aut(R2 ) be defined by α : b a Show that R{α, σ 1 } is a unital subalgebra of End(R2 ). Show that it is proper by giving an example of an endomorphism of R2 not in this subalgebra. Exercise 279 Let V be the space of all real-valued functions on the interval [−1, 1] which are infinitely differentiable, and let δ be the endomorphism of V which assigns to each function f its derivative. Find the kernel and image of δ.


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Exercise 280 Let α : C → C be the function defined by α : a + bi → −b + ai. Is α an endomorphism of C considered as a vector space over R? Is it an endomorphism of C considered as a vector space over itself ? Exercise 281 Let V be a vector space of finite dimension n over a field F and let α ∈ End(V ). Show that there exists an automorphism β of V satisfying αβα = α. Exercise 282 Let V = M2×2 (R), which is a vector space over R. Consider the function α : V → V defined by ! ! |a11 | |a12 | a11 a12 → . α: a21 a22 |a21 | |a22 | Is α an endomorphism of V ? Exercise 283 Consider R as a vector space over Q and let α be an endomorphism of this space satisfying the condition that there exists an a0 ∈ R such that α is continuous at a0 . Show that α is continuous at every a ∈ R. Exercise 284 Let A be a nonempty set and let V be the collection of all subsets of A, considered as a vector space over GF (2). For which subsets C of A is the function B → B ∪ C an endomorphism of V ? Exercise 285 Let V be a vector space of finite dimension n over a field F and let {αij | 1 ≤ i, j ≤ n} be a collection of endomorphisms of V, not all of which are equal to σ 0 , satisfying the condition that

αih if j = k αij αkh = . σ 0 otherwise Show that there exists a basis {v1 , . . . , vn } of V such that

vj if i = k αjk (vi ) = . 0V otherwise Exercise 286 Let V be a vector space of finite dimension n over a field F and choose an element α ∈ End(V ). Let ϕ : End(V ) → End(V ) be the function defined by β → βα. This is an endomorphism of End(V ), considered as a vector space over F. Show that a positive integer n satisfies αn = σ 0 if and only if ϕn is the 0-function. Exercise 287 Let α be an endomorphism of R3 satisfying the condition that α2 = σ 0 . Show that there exists a linear transformation β : R3 → R and that there exists a vector y ∈ R3 satisfying α(v) = β(v)y for all v ∈ R3 .

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Exercise 288 For each 0 = a ∈ R, let β a : C → C be the function defined by β a : z → z + az. Show that β a is an endomorphism of C considered as a vector space over R, and describe its image and kernel. Exercise 289 Let V be a vector space finitely generated over Q and let α, β ∈ End(V ) satisfy 3α3 + 7α2 − 2αβ + 4α − σ 1 = σ 0 . Show that αβ = βα. Exercise 290 Let V be as vector space over a field F and let α, β, γ ∈ End(V ) satisfy αβ = σ 1 = αγ. Show that βγ = γβ. Exercise 291 Let F be a field of characteristic other than 2 and let V be a vector space of finite dimension n over F. Let α be an endomorphism of V satisfying the condition that α2 = σ 1 . Show that rk(σ 1 − α) + rk(σ 1 + α) = n. Exercise 292 Let V be a vector space over a field F which is not finitely generated, and let σ 0 = α ∈ End(V ). Set A = {β ∈ End(V ) | αβ = σ 1 }. Show that if A has more than one element then it is infinite. Exercise 293 Let V be a vector space over a field F having dimension greater than 1. Show that there exists a function α ∈ V V which is not an endomorphism of V but which nonetheless satisfies the condition that α(av) = aα(v) for all a ∈ F and all v ∈ V. Exercise 294 Let V be a vector space over a field F satisfying the condition that αβ = βα for all α, β ∈ End(V ). Show that dim(V ) = 1. Exercise 295 Let V = M2×2 (R), considered as a vector space over R. Let α : V → V be the function defined by ! ! a b a + 2b + c + 2d 2a + 4b + 3c + 5d α: → . c d 3a + 6b + 2c + 5d a + 2b + c + 2d Is α an endomorphism of V ? Is it an automorphism of V ? Exercise 296 Let V be the vector space of all continuous functions from R ( 2 to itself and )let α : V → V be the function defined by α : f (x) → x + sin(x) + 2 f (x). Show that α is an automorphism of V. Exercise 297 Let F be a field and let α : F [X] → F [X] be the function defined by α : p(X) → p(X + 1). Is α an endomorphism of F [X]? Is it an automorphism? Exercise 298 Let F be a field and, for each a ∈ F, let θ a be the endomorphism of F [X] defined by θa : p(X) → p(X + a). Let α ∈ End(F [X]) satisfy α(X) ∈ F and αθa = θa α for all a ∈ F. Can α be a monomorphism?


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

   a a − 2b  . Is c Exercise 299 Let α ∈ End(R3 ) be defined by α :  b  →  c a−b α an automorphism of R3 ? Exercise 300 Let α be the endomorphism of R(∞) defined by α : [a1 , a2 , a3 , . . .] → [b1 , b2 , b3 , . . .], where bh = j≤h (−1)j−1 h−1 j−1 aj for each h ≥ 1. Show that α is an automorphism satisfying α = α−1 . Exercise 301 Let V be a vector space finitely generated over R and let α be an endomorphism of V satisfying α3 + 4α2 + 2α + σ 1 = σ 0 . Show that α ∈ Aut(V ). Exercise 302 Let V be a vector space over a field F and let α, β ∈ End(V ) satisfy αβ = σ 1 . Set ϕ = σ 1 − βα. Show that for every integer n−1 n ≥ 1 we have σ 1 = k=0 β k ϕαk + β n αn . Exercise 303 Let V be the space of all polynomial functions from the interval [0, 1] on the real line to R. Let α and β be the endomorphisms 41 4x of V defined by α(f ) : x → 0 f (t)dt and β(f ) : x → x f (t)dt. Find im(α + β). Is it true that αβ = βα? be a field and let V = F ∞ . Let n > 1 be an   d1   integer. Each vector y =  ...  ∈ F n defines an endomorphism θy Exercise 304 Let F

dn

n of V by θy : [a1 , a2 , . . .] → [b1 , b2 , . . .], where bh = i=1 ah−1+i di , for h = 1, 2, . . . . Show that if θy is a monomorphism then the polynomial n p(X) = i=1 di X i−1 ∈ F [X] has no roots in F. Exercise 305 Let F = GF (5) and let V = F 3 . How many endo    1 2 morphisms α of V satisfy the conditions α  0  =  1  and 0 0     0 1 α  3  =  1 ? 0 1 Exercise 306 Let V be the set of all continuous functions from R to itself, which is a vector space over R. Let α : V → V be the function defined by α(f ) : x → f x2 for all x ∈ R and all f ∈ V. Is α an automorphism of V ?

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Exercise 307 Let V = R∞ and let W be the subspace of V consisting of all convergent sequences. Let α ∈ End(V ) be defined by h 1 for all h ≥ 1. If α : [a1 , a2 , . . .] → [b1 , b2 , . . .], where bh = h i=1 ai v ∈ V satisfies α(v) ∈ W, is v itself necessarily in W ? Exercise 308 Let V be a vector space over a field F and , let α ∈ k Aut(V ). Let W1 , . . . , Wk be subspaces of V satisfying V = i=1 Wi . ,k For each 1 ≤ i ≤ k, let Yi = {α(w) | w ∈ Wi }. Is V = i=1 Yi ? Exercise 309 Consider R as a vector space over Q. An endomorphism of this space is bounded if and only if there exists a nonnegative real number m(α) satisfying the condition that |α(x)| ≤ m(α)|x| for all x ∈ R. Does the set of all bounded endomorphisms of R form an R-subalgebra of End(R)? Exercise 310 Let F be a field, let n be a positive integer, and let V = Mn×n (F ). Given a matrix B ∈ V, is the function αB : V → V defined by αB : A → AB + BA an endomorphism of V ? Exercise 311 Let F be a field and let V = F [X]. Let δ ∈ End(V ) be the formal differentiation function and let α ∈ End(V ) be defined by α : p(X) → Xp(X). Show that αδ − δα = σ 1 . Exercise 312 Let V be a nontrivial vector space over a field F. Is the set of all automorphisms of V a subspace of the vector space End(V ) over F ? Exercise 313 Consider GF (3) as a vector space over itself. Does there exist an automorphism of this space other than σ 1 ? Exercise 314 Let V = F ∞ for some field F. Each w = [c1 , c2 , . . .] ∈ V defines a function β w : V → V by β w : [a1 , a2 , . . .] → [a1 , a1 c1 + a2 , (a1 c1 + a2 )c2 + a3 , . . .]. Show that β w is an automorphism of V. Exercise 315 Let V be a vector space over a field F ; let α ∈ End(V ) and let β ∈ Aut(V ). Define the function θ : V 2 → V 2 by setting ! ! β(v) v → . Is θ necessarily an automorphism of V 2 ? θ: α(v) + v v Exercise 316 Let F = GF (5) and let α ∈ Aut(F 2 ) be defined by ! ! a 2b α : → . Show that there exists a positive integer h b a + 2b satisfying αh+1 = α and find the smallest such integer h.


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Exercise 317 Let F be a field of characteristic other than 2. Let V be a vector space over F and let α, β, γ, δ be endomorphisms of V satisfying the condition that α − β and α + β are automorphisms of V. Show that there exist endomorphisms ϕ and ψ of V satisfying ϕα + ψβ = γ and ψα + ϕβ = δ. Exercise 318 Let V be a vector space of finite dimension n over a field F. Let α ∈ End(V ) and assume that there exists a vector in y ∈ V satisfying the condition that D = {α(y), α2 (y), . . . , αn (y)} is a basis for V. Show that D = {y, α(y), . . . , αn−1 (y)} is also a basis for V and that α ∈ Aut(V ). Exercise 319 Let F be a field and let V = F (Z) . Let α be the endomorphism of V defined by α(f ) : i → f (i + 1) for all f ∈ V. Show / Aut(V ) for all 0 = c ∈ F. that α − cσ 1 ∈ Exercise 320 Let V be a vector space of finite dimension n over a field F , and let 0 < k ≤ n be a positive integer. Let Ak be the set of all subspaces of V having dimension k. Let α ∈ Aut(V ) and, for each W ∈ Ak , let θα (W ) = {α(w) | w ∈ W }. Show that the function θα is a permutation of Ak . Exercise 321 Let r, s, and t be distinct real numbers and let α be     a a + br + cr2 the endomorphism of R3 defined by α :  b  →  a + bs + cs2  . Is a + bt + ct2 c 3 α an automorphism of R ? Exercise 322 Let V be a vector space over a field F and let α ∈ ∞ End(V ). Show that W = i=1 ker(αi ) is a subspace of V which is invariant under α. Exercise 323 Let α and β be    a 2a − 2b − 2c − 2d  b   5b − c − d   α:  c  →  −b + 5c − d d −b − c + 5d

the endomorphisms of Q4 defined by     a 0   b   −b + 2c + 3d  and β :      c  →  2b − 3c + 6d d 3b + 6c + 2d

  . 

Find two nontrivial proper subspaces of Q4 which are invariant both under α and under β. Exercise 324 Let F be a field and let V = F 4 . Let α be the endomor    a a−b  b   a−b     phism of V defined by α :   c  →  a − b  . Does there exist a d c−b−d two-dimensional subspace of V invariant under α?

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Exercise 325 Let V be a vector space over a field F and let α ∈ End(V ). If W and Y are subspaces of V which are invariant under α, show that both W + Y and W ∩ Y are invariant under α. Exercise 326 Let W be a subspace of a vector space V over a field F and let S be the set of all α ∈ End(V ) such that W is invariant under α. Is S necessarily an F -subalgebra of End(V )? Exercise 327 Let V be a vector space over a field F and let α ∈ End(V ). If W is a subspace of V, show that the set of all subspaces of W which are invariant under α, partially ordered by inclusion, has a maximal element. of V consisting Exercise 328 Let V = R∞ and let W be the subspace ∞ a converges. Let of all sequences [a1 , a2 , . . .] for which the series i i=1 σ be a permutation of the set of( all positive integers and let α ∈ End(V ) ) be defined by α : [a1 , a2 , . . .] → aσ(1) , aσ(2) , . . . . Is W invariant under α? Exercise 329 Let V and let α ∈ End(V ). satisfying α(x0 ) = cx0 that F {x0 , x1 , . . . , xn }

be a vector space over a field F. Let 0 = c ∈ F Let {x0 , x1 , . . . , xn } be a set of vectors in V and α(xi ) − cxi = xi−1 for all 1 ≤ i ≤ n. Show is a subspace of V which is invariant under α.

Exercise 330 Let F be a field which is not finite and let V be a vector space over F having dimension greater than 1. For each 0 = c ∈ F, show that there exist infinitely-many distinct subspaces of V which are invariant under the endomorphism σ c of V. Exercise 331 Let α and β be endomorphisms of a vector space V over a field F and let θ ∈ Aut(V ) satisfy θα = βθ. Show that a subspace W of V is invariant under α if and only if W = {θ(w) | w ∈ W } is invariant under β. Exercise 332 Let α and β be endomorphisms of a vector space V over a field F satisfying αβ = βα. Is ker(α) invariant under β? Exercise 333 Let V be a vector space over a field F and let α ∈ End(V ) be a projection. Show that σ 1 − α is also a projection. Exercise 334 Let V be a vector space finitely generated over a field F and let α ∈ End(V ) satisfy the condition α2 (σ 1 − α) = σ 0 . Is α necessarily a projection? Exercise 335 Let V be the space of all continuous functions from R to itself and let W = R{sin(x), cos(x)} ⊆ V. Let δ be the endomorphism of W which assigns to each function its derivative. Find a polynomial p(X) ∈ R[X] of degree 2 satisfying p(δ) = σ 0 .


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Exercise 336 Let V be a vector space having finite dimension over Q and assume that there exists an α ∈ Aut(V ) satisfying α−1 = α2 + α. Show that dim(V ) is divisible by 3. Exercise 337 Let n be a positive integer and let        a1  ..  n G =  .  ∈ R ai ≥ 0 for all 1 ≤ i ≤ n .     an Let α be an endomorphism of Rn satisfying the condition that α(v) ∈ G implies that v ∈ G. Show that α ∈ Aut(Rn ). Exercise 338 Let V be a vector space over a field F and let W and Y be subspaces of V satisfying W + Y = V. Let Y be a complement of Y in V and let Y be a complement of W ∩ Y in W. Show that Y ∼ = Y . Exercise 339 Let F be a field of characteristic other than 2 and let V be a vector space over F. Let α,β ∈ End(V ) be projections satisfying the condition that α + β is also a projection. Show that αβ = βα = σ 0 . Exercise 340 Let V be a vector space over F and let α,β ∈ End(V ). Show that α and β are projections satisfying ker(α) = ker(β) if and only if αβ = α and βα = β. Exercise 341 Let V be a vector space finitely generated over a field F and let α = σ 1 be an endomorphism of V which is a product of projections. Show that α ∈ / Aut(V ). Exercise 342 Let V be a vector space over Q and let α ∈ End(V ). Show that α is a projection if and only if (2α − σ 1 )2 = σ 1 . Exercise 343 Let α and β be endomorphisms of a vector space V over a field F and let f (X) ∈ F [X] satisfy f (αβ) = σ 0 . Set g(X) = Xf (X). Show that g(βα) = σ 0 . Exercise 344 Let V = RR and let g ∈ V. Find necessary and sufficient conditions on g for the endomorphism f → gf of V to be a projection. Exercise 345 Let W be a subspace of a vector space V over a field F which is invariant under an endomorphism α of V. Let β ∈ End(V ) be a projection satisfying the condition that im(β) = W. Show that βαβ = αβ. Exercise 346 Let V be a vector space of finite dimension n over a field F and let α ∈ End(V ). Show that there exists an automorphism β of V and a projection θ of V satisfying α = βθ.

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Exercise 347 Let F be a field of characteristic other than 2 and let V be a vector space over F. Let α ∈ End(V ) be a projection satisfying the condition that α − β is a projection for all β ∈ End(V ). Show that α = σ1 . Exercise 348 Let V be a vector space over F and let α,β ∈ End(V ) be projections satisfying the condition that im(α) and im(β) are disjoint. Is it necessarily true that αβ = βα? Exercise 349 Let V be a vector space of finite dimension n over a field F and let S = End(V ) Aut(V ). For α, β ∈ S, show that im(α) = im(β) if and only if {aθ | θ ∈ S} = {βϕ | ϕ ∈ S}. Exercise 350 Let F be a field. Does there exist an endomorphism α of F 3 which is not a projection satisfying the condition that α2 is a projection equal neither to σ 0 nor to σ 1 . Exercise 351 Let V be a vector space finite dimensional over a field F and let α be an endomorphism of V. Show that there exist a positive integer k such that im(αk ) and ker(αk ) are disjoint. Exercise 352 Let F be a field of characteristic other than 2, and let V be a vector space over F. Let α ∈ End(V ) satisfy α3 = α. Show that V = W1 ⊕ W2 ⊕ W3 , where W1 = {v ∈ V | α(v) = v}, W2 = {v ∈ V | α(v) = −v}, and W3 = ker(α). Exercise 353 Let F be a field of characteristic other than 2 and let V be a finitely-generated vector space over F. Show that every endomorphism of V is the sum of two automorphisms of V. Exercise 354 Let n > 1 be an integer and let θ : Rn → R be the   a1 n   function defined by θ :  ...  → i=1 a2i . Assume that we can define an an operation • on R satisfying the condition that (Rn , •) is an associative unital R-algebra with multiplicative identity e, and also satisfying the condition that θ(v•w) = θ(v)θ(w) for all v, w ∈ Rn . Show that (Rn , +, •) is a division algebra over R. n

Exercise 355 Any sequence v = [a1 , a2 , . . .] ∈ R∞ defines an endomorphism αv of R[X] which acts on elements n of the canonical basis of R[X] according to the rule αv : X n → k=0 nk (k!)ak+1 X n−k for each nonnegative integer n. Given a ∈ R, find v, w ∈ R∞ such that αv : p(X) → p(X + a) and αw : p(X) → p(X + a) − p(a).

8 Representation of linear transformations by matrices

In this chapter we show how we can study linear transformations between finitely-generated vector spaces by studying matrices1 . Let V and W be finitely-generated vector spaces over a field F, where dim(V ) = n and dim(W ) = k. Fix bases B = {v1 , . . . , vn } of V and D = {w1 , . . . , wk } of W. From Proposition 5.4, we know that if we are given a linear transformation α ∈ Hom(V, W ) then for each 1 ≤ j ≤ n there exist scalars k a1j , . . . , akj satisfying the condition α(vj ) = i=1 aij wi , and that these scalars are in fact uniquely determined by α. Thus α defines a matrix [aij ] ∈ Mk×n (F ). Conversely, assume we have a matrix A = [aij ] ∈ Mk×n (F ). Then we know that n every vector v in V can be written in a linear transa unique way in the form j=1 bj vj and so A defines k n wi . a b formation α ∈ Hom(V, W ) by setting α : v → i=1 ij j j=1 Moreover, it is clear that different linear transformations in Hom(V, W )

1 The theory of matrices and their relation to linear transformations was developed in detail by the 19th-century British mathematician Sir Arthur Cayley, one of the most prolific researchers in history.

117

118

8. Representation of linear transformations by matrices

define different matrices in Mk×n (F ) and different matrices in Mk×n (F ) define different linear transformations in Hom(V, W ). We summarize the above remarks in the following proposition. (8.1) Proposition: Let V be a vector space of finite dimension n over a field F and let W be a vector space of finite dimension k over F. For every basis B of V and every basis D of W there exists a bijective function ΦBD : Hom(V, W ) → Mk×n (F ), which is an isomorphism of vector spaces over F. Proof: We have already seen that if B = {v1 , . . . , vn } and D = {w1 , . . . , wk }, then the function ΦBD is defined by ΦBD (α) = [aij ], k where α(vj ) = i=1 aij wi for all 1 ≤ j ≤ n, and that this function is bijective. We are therefore left to show that this is a linear transformation. Indeed, if ΦBD (α) = [aij ] and ΦBD (β) = [bij ] then

(α + β)(vj ) =

k i=1

(aij + bij )wi =

k i=1

aij wi +

k

bij wi = α(vj ) + β(vj )

i=1

for all 1 ≤ j ≤ n, and so ΦBD (α + β) = ΦBD (α) + ΦBD (β). Similarly, k k if c ∈ F then (cα)(vj ) = i=1 caij wi = c i=1 aij wi = c (α(vj )) for all 1 ≤ j ≤ n, and so ΦBD (cα) = cΦBD (α). Thus we see that ΦBD is indeed a linear transformation and thus also an isomorphism. We have already seen that, in the above situation, dim(Mk×n (F )) = kn and so, by Proposition 6.9, we also see that dim(Hom(V, W )) = kn. Example: Let V = R3 and let B be the canonical basis on V. Each   a1 vector v =  a2  ∈ V defines a linear transformation αv : V → V a3   0 −a3 a2 0 −a1  . given by αv : w → v × w. Then ΦBB (αv ) =  a3 −a2 a1 0 Example: Let V = R3 and W = R2 . Choose bases       0.5 0.5 0   B =  −0.5  ,  0  ,  0.5    0 −0.5 0.5


of V and of D =

1 1

! ,

1 0

!-

119



 r of W. If  s  ∈ R3 then there t

exist b1 , b2 , b3 ∈ R satisfying           b1 + b2 r 0.5 0.5 0 1  s  = b1  −0.5  + b2  0  + b3  0.5  =  −b1 + b3  2 −b2 + b3 t 0 −0.5 0.5 and so we have to solve the system of linear equations 2r = b1 + b2 2s = −b1 + b3 2t = −b2 + b3

and if we do so, we get b1 = r − s!+ t, b2 = r + s − t, and b3 = r + s + t. 3 5 7 defines a linear transformation α ∈ The matrix A = 4 8 2 Hom(V, W ) given by       0.5 0.5 0 α : b1  −0.5  + b2  0  + b3  0.5  → 0 −0.5 0.5 ! ! 1 1 (3b1 + 5b2 + 7b3 ) + (4b1 + 8b2 + 2b3 ) . 1 0 so



 r α  s  t

= (15r + 9s + 5t) =

29r + 15s + 3t 15r + 9s + 5t

1 1 !

! + (14r + 6s − 2t)

1 0

!

.

It is very important to emphasize that the matrix representation of a linear transformation depends on the bases which we fixed at the beginning, and on the order in which the elements of the bases are written! If we choose different bases or write the elements of a chosen basis in a different order, we will get a different matrix. Shortly, we will consider the relation between the matrices which represent a given linear transformation with respect to different bases. Let V be a vector space finitely generated over a field F, let α be an endomorphism of V, and let W be a subspace of V which is invariant under α. As we have already seen, the restriction β of α to

120


W is an endomorphism of W. Now, let B = {v1 , . . . , vk } be a basis for W, which we can expand to a basis D = {v1 , . . . , vn } for all of V. If k ΦDD (α) = [aij ] then for all 1 ≤ j ≤ k we have α(vj ) = i=1 aij vi and so aij = 0 whenever 1 ≤ j ≤ k and k < i ≤ n. Thus we see that the ! A11 A21 matrix ΦDD (α) is of the form , where A11 = ΦBB (β). O A22 The subspace Y = F {vk+1 , . . . , vn } of V is a complement of W in V. If it too is invariant under α then we would also have A21 = O and so α is represented by a matrix composed of two square matrices “strung out” along the diagonal. From a computational point of view, such a representation has distinct advantages. Beside addition and scalar multiplication of matrices, we can also define the product of two matrices, provided that these matrices are of suitable sizes. Let (K, •) be an associative unital algebra over a field F. If A = [vij ] ∈ Mk×n (K) and B = [wjh ] ∈ Mn×t (K) for some positive integers k, n, and t, we define the matrix AB to be the matrix [yih ] ∈ M k×t (K) where, for each 1 ≤ i ≤ k and all 1 ≤ h ≤ t, we n set yih = j=1 vij • wjh . For the most part, we will be interested in this construction for the case K = F, but sometimes we will have need of the more general construction. Note that a necessary condition for the product of two matrices to be defined is that the number of columns in the first matrix be equal to the number of rows in the second matrix. 2 3 2 −1 2 1

Example: If A =

! ∈ M2×3 (Q) and



 −1 0 2 −1 B =  1 0 1 −2  ∈ M3×4 (Q) 2 1 0 −3 then AB =

5 2 7 5 1 0

−14 −6

! ∈ M2×4 (Q) but BA is not defined.

Example: If we consider the matrices A =   −1 0 and B =  1 0  ∈ M3×2 (Q) then AB = 2 1   −2 −3 −2 3 2  ∈ M3×3 (Q). BA =  2 3 8 5

2 −1 5 5

! 3 2 ∈ M2×3 (Q) 2 1 ! 2 ∈ M2×2 (Q) and 1


121



 b1   Suppose that A = [aij ] ∈ Mk×n (F ) and v =  ...  ∈ F n . Then bn   c1 n   Av =  ...  ∈ F k where, for each 1 ≤ i ≤ k, we have ci = j=1 aij bj . ck Denoting the columns of A by u1 , . . . , un , we see that Av =

n

j=1 bj uj .

So we conclude that if there exists a nonzero vector v such that Av =  0  ..   .  , then the columns of A must be linearly dependent. If every 0 element of F k is of the form Av for some v ∈ F n , then the columns of A must form a generating set for F k . Let (K, •) be an associative F and let n  algebra over   unital  a field v1 w1     be a positive integer. If v =  ...  and w =  ...  are elements of vn wn n K n then v T w = [ i=1 vi • wi ] ∈ M1×1 (K). This is called the interior productof v and w. This 1 × 1 matrix is usually identified with the n scalar i=1 vi • wi ∈ K, which we will denote by v w, in a departure from usual notation2 . Dually, the exterior product of v and w is defined to be the matrix vwT = [yij ] ∈ Mn×n (K), where yij = vi •wj . We will denote the exterior product of v and w by v ∧ w. Notice that the exterior product is not commutative, but rather v ∧ w = (w ∧ v)T . Exterior products of vectors are encountered far less often than interior products, but have important applications in many areas, among them physics (in the Dirac model of quantum physics, interior products are called bra-ket products, whereas exterior products are called ket-bra products).

In particular, we note the following: let K be an algebra over a field F , let A ∈ Mk×n (K), and let B ∈ Mn×t (K). Let v1T , . . . vkT be the rows of A and let w1 , . . . , wt be the columns of B. Then AB = [cij ], where cij = vi wj for all 1 ≤ i ≤ k and all 1 ≤ j ≤ t. 2 The usual notation is v · w, but that can cause confusion with the dot product, which we will study later, in the case that F = C. For that reason, also, we use the term “interior product” rather than the often-seen “inner product”.

122




 a1   Let F be a field, let n be a positive integer, let v =  ...  and an   ba1   w =  ...  belong to F n , and let C = [cij ] ∈ Mn×x (F ). Then the bn computation of v Cw =

n

n j=1 cij bj

requires n2 + n multipli  u1   cations and n2 −1 additions. However, if we can find vectors u =  ...  

i=1 ai

un



y1  ..  and y =  .  in F n such that C = u ∧ y, then, by the distributive nn n n n n = ( and u y b a u ) y b law, v Cw = i=1 ai i j j i i j j j=1 i=1 j=1 this requires only 2n + 1 multiplications and 2n − 2 additions. Similarly, if we can find vectors u, u , y, y ∈ F n such that C = u ∧ y + u ∧ y , then the computation of v Cw requires 4n + 2 multiplications and 4n − 4 additions. For large values of n, this can result in considerable saving, especially if the computation is to be repeated frequently. Example: Combinatorial optimization is the area of mathematics dealing with the computational issues arising from finding optimal solutions to such problems as the traveling salesman problem, testing Hamiltonian graphs, sphere packing, etc. The general form of combinatorial optimization problems is the following: let F be a subfield of R and let n be a positive integer. Assume that we have a nonempty finite (and in general very large) subset S of Nn ⊆ F n . Usually, the set S arises from the characteristic functions of certain subsets of {1, . . . , n} of interest in   a1   the problem. Then, given a vector v =  ...  ∈ F n , we want to find an min {s v | s ∈ S} . Note that if we consider F not as a subset of R but as a subset of the optimization algebra R∞ , then the problem becomes one of computing p(a1 , . . . , an ), where

p(X1 , . . . , Xn ) =

  

X1i1 · . . . · Xnin

 

  

  i1   ..  ∈ S  .   in


123

is a polynomial in several indeterminates over R∞ (polynomials with coefficients in a semifield are defined in the same way as polynomials with coefficients in a field). Observe that multiplying a k × n matrix by an n × t matrix requires kt(n − 1) arithmetic operations. If these numbers are all very large, as is often the case in real-life applications of matrix theory, the computational overhead – and risk of accumulated errors due to rounding and truncation – is substantial.3 We will keep this in mind throughout our discussion, and try to consider strategies of minimizing this risk. In this connection, we should note that the product of two matrices has an important property: let (K, •) be an associative unital algebra over a field F assume that A = [vij ] ∈ Mk×n (K) and B = [wij ] ∈ Mn×t (K), where k, n, and t are positive integers. Furthermore, let us pick positive integers 1

= k(1) < k(2) < . . . < k(p + 1) = k

1 1

= n(1) < n(2) < . . . < n(q + 1) = n = t(1) < t(2) < . . . < t(r + 1) = t.

For all 1 ≤ i ≤ p and all 1 ≤ j ≤ q, let  ... vk(i),n(j+1) vk(i),n(j)  . .. .. Aij =  . vk(i+1),n(j)

...

  .

vk(i+1),n(j+1) 

A11  This allows us to write A in block form  ... Ap1

... ...

 A1q ..  . Note .  Apq

that these blocks are not necessarily square matrices. In the same way,   B11 . . . B1t  .. ..  . Then AB = we can write B as a matrix  . .  Bq1 . . . Bqt  C1t ..  where, for each 1 ≤ i ≤ p and each 1 ≤ h ≤ t, .  . . . Cpt q we have Cih = j=1 Aij Bjh . A sophisticated use of this method can



C11  ..  . Cp1

...

3 We will often mention large matrices, without being too specific as to what that means. As a rule of thumb, a matrix is “large”, and calls for special treatment as such, when it cannot be stored in the RAM memory of whatever computer we are using for our computations. Such matrices occur in sufficiently-many applications that considerable research is devoted to dealing with them.

124


substantially decrease the number of operations needed to multiply two matrices, as we shall see.

Needless to say, this seemingly odd definition of the product of two matrices was not chosen at random4 . Indeed, it satisfies certain important properties. Thus, if (K, •) is an associative unital algebra over a field F , if k, n, t, and p are positive integers, and if we have matrices A ∈ Mk×n (K), B, B1 , B2 ∈ Mn×t (K), and C ∈ Mt×p (K), then (1) A(BC) = (AB)C; (2) A(B1 + B2 ) = AB1 + AB2 ; (3) (B1 + B2 )C = B1 C + B2 C. As a consequence, we see that if B ∈ Mn×t (K) is given, then the function from Mk×n (K) to Mk×t (K) defined by A → AB is a linear transformation of vector spaces. We also note that if A = [vij ] ∈ Mk×n (K) and B = [wjh ] ∈ Mn×t (K), T T then AT ∈ Mn×k (K) and B T ∈ M nt×n (K) so B A ∈ Mt×k (K). T T Indeed, B A = [yhi ], where yhi = j=1 wjh • vij . Hence, if K is also commutative (and in particular if K = F ), we have B T AT = (AB)T .

The definition of matrix multiplication is in fact a direct consequence of the relation between matrices and linear transformations, which we have already observed. This is best seen in the following result.

(8.2) Proposition: Let V be a vector space of finite dimension n over a field F for which we have chosen a basis B = {v1 , . . . , vn }, let W be a vector space of finite dimension k over F for which we have chosen a basis D = {w1 , . . . , wk }, and let Y be a vector space of finite dimension t over F, for which we have chosen a basis E = {y1 , . . . , yt }. If α ∈ Hom(V, W ) and β ∈ Hom(W, Y ) then ΦBE (βα) = ΦDE (β)ΦBD (α).

4 Matrix multiplication was first defined by the 19thcentury French mathematician Jacques Philippe Binet. It took some getting used to; many decades later, the father of astrophysics, Sir Arthur Eddington, still wrote “I cannot believe that anything so ugly as multiplication of matrices is an essential part of the scheme of nature”.


125

Proof: Assume that ΦBD (α) = [aij ] and ΦDE (β) = [bhi ]. Then α : v →

k n

cj aij wi and βα : v →

i=1 j=1

k t n

cj bhi aij yh ,

h=1 i=1 j=1

showing the desired equality.

We can extend the definition of matrix multiplication as follows: let h, k, and n be positive integers and let V be a vector space over a field F. If A = [aij ] ∈ Mh×k (F ) and if M = [vjt ] ∈ Mk×n (V ), we can define k AM ∈ Mh×n (V ) to be the matrix [uit ], where uit = j=1 aij vjt for all 1 ≤ i ≤ h and 1 ≤ t ≤ n. Notice that if A, B ∈ Mk×k (F ) and if M, N ∈ Mk×n (V ) then (1) A(BM ) = (AB)M ; (2) A(M + N ) = AM + AN ; (3) (A + B)M = AM + BM. In general, and especially when we are talking of actual computations, it is easier to work with matrices than with linear transformations, and indeed most of the modern computer software and hardware are designed to facilitate easy and speedy matrix computation. Therefore, given finitelygenerated vector spaces V and W over a field F, it is usual to fix bases for them and then identify Hom(V, W ) with the space of all matrices over F of the appropriate size. The choice of the correct bases then becomes critical, and we will focus on that throughout the following discussions. Such a choice usually depends on the problem at hand. In particular, the automatic choice of canonical bases, when they exist, may not be the best for a given problem, and can entail a considerable cost both in computational time and numerical accuracy.

Exercises Exercise 356 Let V be the vector space over R composed of all polynomials in R[X] having degree less than 3 and let W be the vector space over R composed of all polynomials in R[X] having degree less than 4. Let α : V → W be the linear transformation defined by α : a + bX + cX 2 → (a + b) + (b + c)X + (a + c)X 2 + (a + b + c)X 3 . Select bases

B = {1, X + 1, X 2 + X + 1} for V and D = {X 3 − X 2 , X 2 − X, X − 1, 1}

for W. Find the matrix ΦBD (α).

126


a b c d

Exercise 357 Let K = M2×2 (R) and let A =

! ∈ K. Let D be

the canonical basis of K. If α, β ∈ End(K) are defined by α : X → XA and β : X → AX, find ΦDD (α) and ΦDD (β). 

 0 1 2 3 Exercise 358 Given the matrix A =  1 3 4 0  ∈ M3×4 (R), find 3 2 0 1   1 0 0 the set of all matrices B ∈ M4×3 (R) satisfying AB =  0 1 0  . 0 0 1 

 1 8 Exercise 359 Given the matrix A =  3 5  ∈ M3×2 (Q), 2 2  1 0 0 of all matrices B ∈ M2×3 (Q) satisfying AB =  0 1 0 0 0 1 1 the set of all matrices C ∈ M2×3 (Q) satisfying CA = 0

find the set   and find 0 1

! .



 −1 2 1 2   ∈ M4×3 (R), 3 1  1 −1   1 0 0 find the set of all matrices B ∈ M3×4 (R) satisfying BA =  0 1 0  . 0 0 1 1  0 Exercise 360 Given the matrix A =   −1 2

Exercise   361 Find the a a+b+c α :  b  → b+c c      0 3  −1  0  ,  1  ,  −1  2 1 0 Exercise 362  0  0 condition   0 0

matrix representing the linear transformation ! from R3 to R2 with respect to the bases 

 3  of R and 

Find the set of all matrices   1 0 0 0 1  0 1 0   0 0 A = A 0 0 1  0 0 0 0 0

−1 1

! ,

1 0

!of R2 .

A ∈ M4×3 (R) satisfying the  0 1 . 0


127

Exercise 363 Let α be an endomorphism of R3 represented with respect   0 2 −1 to some basis by the matrix  −2 5 −2  . Is α a projection? −4 8 −3 Exercise 364  1  1   1 ∗

Find the real numbers missing from the   −3 −25 −1 !  −1 ∗  −1 ∗ 7 ∗ ∗  =  ∗ ∗  ∗ 1 ∗ 0 ∗ 1 ∗ ∗

following equation:  1 3 ∗ ∗  . 5 ∗  ∗ 0



   a 3a + 2b Exercise 365 Let α :  b  →  −a − c  be an endomorphism of c a + 3b R3 . Find the matrix representing α with respect to the basis B =       1 1 0    −1  ,  0  ,  1  of R3 .   0 −1 0 Exercise 366 Let D = {v1 , v2 , v3 } be a basis for R3 and let α be   −1 −1 −3 the endomorphism of R3 satisfying ΦDD (α) =  −5 −2 −6  . Find 2 1 3 ker(α). Exercise 367 Let V be the subspace of R[X] consisting of all polynomials of degree less than 3 and choose the basis B = {1, X, X 2 } for V.   1 1 1 Let α ∈ End(V ) satisfy ΦBB (α) =  0 2 2  . Let D be the basis 0 0 3 {1, X + 1, 2X 2 + 4X + 3} for V. What is ΦDD (α)? Exercise 368 Let α ∈ End(R3 )  2 2 ical basis by the matrix  1 1 1 1 α is represented with 

0 0 by the matrix  0 1 0 0

be represented with respect to the canon 0 2  . Find a real number a such that 2       a −2 1    −1  ,  a  ,  1  respect to the basis   0 1 a  0 0 . 4

128


Exercise 369 Let V be the subspace of R[X] consisting of all polynomials of degree less than 3 and let α ∈ End(V ) be defined by α : aX 2 + bX + c → (a + 2b + c)X 2 + (3a − b)X + (b + 2c). Find ΦDD (α), where D = {X 2 + X + 1, X 2 + X, X 2 }. Exercise 370 Find all rational numbers a for which there exists a nonzero     0 0 0 a 1 1  0 0 0   matrix B ∈ M4×3 (Q) satisfying B  1 1 a  =   0 0 0 . 1 a 1 0 0 0 Exercise 371 For which real numbers a does there exist a real number   ! b −1 ! 1 0 a 1 1   1 −1 = b satisfying ? 1 1 a 0 1 1 b Exercise 372 Let V = RR and let W be the subspace of V generated by the linearly-independent set B = {1, x, ex , xex }. Let δ be the endomorphism of W which assigns to each function its derivative. Find ΦBB (δ). Exercise 373 Let B = {1 + i, 2 + i}, which is a basis for C as a vector space over R. Let α be the endomorphism of this space defined by α : z → z. Find ΦBB (α). Exercise 374 Let F = GF (3) and let α : F 3 → F 2   ! a a−b transformation defined by α :  b  → . Let 2a − c c  b !  a a be the linear transformation defined by β : →   2b b 2a

be the linear β : F2 → F4    . Find the 

matrix representing βα with respect to the canonical bases. Exercise 375 Let α ∈ End(R4 ) be represented with respect to the canon  3 −1 0 0  −1 2 −1 0   . Given a vector v ∈ R4 ical basis by the matrix   0 −1 2 −1  0 0 −1 1 satisfying the condition that all entries of α(v) are nonnegative, show that all entries of v are nonnegative.


129

Exercise 376 Let V and W be vector spaces over a field F and choose bases {vi | i ∈ Ω} and {wj | j ∈ Λ} for V and W respectively. Let p : Ω × Λ → F be a function satisfying the condition that the set {j ∈ Λ | p(i, j) = 0} is finite for each i∈ Ω. Let αp : V → W where Γ is a be the function defined as follows: if v = i∈Γ ai vi , are scalars in F, then αp (v) = finite subset of Ω and where the a i a p(i, j)w . Show that α is a linear transformation and that i j p i∈Γ j∈Λ every linear transformation from V to W is of this form. Exercise 377 Let k and n be positive integers, let v ∈ Rn , and let A ∈ Mk×n (R). Show that Av = O if and only if AT Av = O. Exercise 378 Let  8 fying AB =  2 −2 Exercise 379 Find  1 fying AB =  −2 0

A ∈ M3×2 (R) and B ∈ M2×3 (R) be matrices satis 2 −2 5 4  . Calculate BA. 4 5 matrices A ∈ M3×2 (R) and B ∈ M2×3 (R) satis 1 1 0 −6  . 1 −2

Exercise 380 Let F be a field and let n be a positive integer. Let W be a nontrivial subspace of the vector space V = Mn×n (F ) satisfying the condition that if A ∈ W and B ∈ V then AB and BA both belong to W. Show that W = V. Exercise 381 Let a, b, c, a , b , c ∈ C satisfy the condition that aa +bb +   a ( ) cc = 2, and let A = I −  b  a b c . Calculate A2 . c Exercise 382 Find a nonzero matrix A in M2×2 (R) satisfying vAv = 0 for all v ∈ R2 . Exercise 383 Let α be the endomorphism of Q4 represented with respect   1 0 1 −1  2 1 2 1   . Find a twoto the canonical basis by the matrix   0 1 6 1  3 1 3 4 dimensional subspace of Q4 which is invariant under α. Exercise 384 Find the set of all matrices A in M3×3 (R) satisfying   0 1 0 A2 =  0 0 0  . 0 0 0

130


Exercise 385 Find the set of all real numbers a such that the endomor  1 a a phism of R3 represented by the matrix  2 2a 4  with respect to 3 a 6 the canonical basis is an automorphism. Exercise 386 Find the set of all real numbers a and b such that the   1 a b endomorphism of R3 represented by the matrix  0 a 1  with respect 0 a 1 to the canonical basis is a projection. Exercise 387 Let n be a positive integer and let F be a field. For each v, w ∈ F n , consider the function τ v,w : F n → F v defined by τ v,w : y → (w y)v (this function is called the dyadic product function). Show that τ v,w a linear transformation. Is the function F n → Hom(V, F v) defined w → τ v,w a linear transformation? Exercise 388 Let k < n be positive integers and let F be a field. Given a matrix A ∈ Mk×n (F ), do there necessarily exist matrices B, C ∈ Mn×k (F ) satisfying the condition that AB = O ∈ Mk×k (F ) and CA = O ∈ Mn×n (F )? Exercise 389 Let A ∈ Mn×n (Q) be a matrix satisfying the condition that if v ∈ Qn is a vector all of the components of which are nonnegative, then all of the components of Av are nonnegative. Are all of the entries in A necessarily nonnegative?

9 The algebra of square matrices

We are now going to concentrate on the algebraic structure of sets of the form Mn×n (K), where n is a positive integer and (K, •) is an associative unital algebra over a field F. From what we have already seen, this is again an associative unital F -algebra, which will not be commutative if n > 1. The additive identity of this algebra is the matrix all of the entries of which equal 0K . The additive inverse of a matrix A = [dij ] ∈ Mn×n (K) is the matrix [−aij ]. The multiplicative identity of Mn×n (K) is the matrix E = [dij ] given by

e if i = j dij = 0 otherwise where e is the multiplicative identity of (K, •). The most important case is, of course, that of K = F. In this case, the additive identity is O and the multiplicative identity is the matrix I = [aij ] defined by

1 if i = j . aij = 0 otherwise If K is a vector space of dimension n over F and if B is a basis of K, then it is straightforward to verify that the function ΦBB : End(K) → Mn×n (F ) is an isomorphism of unital F -algebras. If F is a field and if n is a positive integer then, corresponding to the associative F -algebra Mn×n (F ), we have the Lie algebra Mn×n (F )− . This Lie algebra is called the general Lie algebra defined by F n . 131

132

9. The algebra of square matrices

Example: Let F can also be written in  a11  a 21     a31 a41

be a field and let A = [aij ] ∈ M4×4 (F ). Then A block form as ! !  a13 a14 a12  a22 a23 a24   ! !  ∈ M2×2 (K),  a33 a34 a32 a42 a43 a44

where K = M2×2 (F ). Addition and multiplication of matrices are so defined (and not accidentally!) so that they give the same results whether performed in M4×4 (F ) or in M2×2 (K). We begin by identifying some particularly-important square matrices over a a unital associative F -algebra K, and with them some significant subalgebras of Mn×n (K). Let (K, •) is an associative unital F -algebra and let n be a positive integer. A matrix A = [dij ] ∈ Mn×n (K) is a diagonal matrix if and only if there exist elements c1 , . . . , cn of K such that

ci if i = j . dij = 0K otherwise The matrices O and E are diagonal. Moreover, the sum and product of diagonal matrices are diagonal matrices, and so the set of all diagonal matrices is an F -subalgebra of Mn×n (K). If K is commutative (and, in particular, if K = F ) then this algebra is also commutative. The units of the subalgebra are all diagonal matrices in which each ci is a unit −1  c1 . . . 0K  ..  = .. of K (and hence surely nonzero). In this case,  ... . .  

c−1 1  ..  . 0K

... .. . ...

 0K ..  . .  −1 cn

0K

...

cn

Example: Let F be a field, let (K, •) is an associative unital F algebra, and let n be a positive integer. A matrix A = [aij ] ∈ Mn×n (K) is a scalar matrix if and only if there exists a scalar c ∈ K such that aij = c when i = j and aij = 0K otherwise. We denote this matrix by cE (and, in particular, cI when K = F ). Scalar matrices are surely diagonal matrices, and both O and E are scalar matrices. Moreover, the sum and product of scalar matrices are scalar matrices. If c, d ∈ K then (cE)(dE) = (dE)(cE) and if 0K = c ∈ K is a unit, then (cE)(c−1 E) = E.


133

Hence the set of all scalar matrices over F forms an F -subalgebra of Mn×n (F ), which is in fact a field. The function F → Mn×n (F ) defined by c → cI is a monic homomorphism of F -algebras, and so we can identify F with the subfield of all scalar matrices of Mn×n (F ). Moreover, it is also easy to see that (cI)A = A(cI) = cA for any A ∈ Mn×n (F ). Let (K, •) is an associative unital F -algebra, let n be a positive integer, and let d be a positive integer less than n. A matrix A = [vij ] ∈ Mn×n (K) is a band matrix of width 2d − 1 if and only if aij = 0K whenever |i − j| > d − 1. Thus, the band matrices of width 1   1 2 0 0 0  2 3 1 0 0     are the diagonal matrices. The matrix   0 0 0 0 0  ∈ M5×5 (R)  0 0 0 0 1  0 0 0 4 4 is an example of a band matrix of width 3. The set of band matrices of fixed width is closed under addition and contains O and I, but is not necessarily closed under multiplication, and so is not a subalgebra of Mn×n (K). However, it is closed under scalar multiplication and so is a subspace of the vector space Mn×n (K) over F. Band matrices over F are very important for numerical computations, especially when d is small relative to n. Of particular importance are band matrices of width 3, which are also known as tridiagonal matrices, and have important use in the computation of quadratic splines and in the computation of extremal eigenvalues of matrices. A special type of tridiagonal matrix in M2n×2n (F ), which we will see   O A11 O . . .  O A22 . . . O    again later, is one of the form   , where the Aii ..   . O

...

O

Ann

are 2×2 blocks. Note that this matrix can also be thought of as a diagonal matrix in Mn×n (K), where K = M2×2 (F ). More generally, if d and n are positive integers, then any diagonal matrix in Mn×n (L), where L = Md×d (K), is a band matrix of width 2d − 1 in Mdn×dn (K). Let (K, •) is an associative unital F -algebra and let n be a positive integer. A matrix A = [cij ] ∈ Mn×n (K) is an upper-triangular matrix if and only if cij = 0K whenever i > j. Thus, the matrix   1 2 6 3 7  0 3 1 0 0     0 0 0 0 0  ∈ M5×5 (R) is upper triangular. The set of all upper   0 0 0 0 1  0 0 0 0 4

134


triangular matrices includes the set of diagonal matrices, is closed under addition, and contains O and E. Moreover, it is closed under multiplication, and so is an F -subalgebra of Mn×n (K). In the case that K = F, we see that the dimension of Mn×n (F ) as a vector space over F equals n2 (n + 1). Upper-triangular matrices arise naturally in many applications, as we will see below. In a similar manner, we say that a matrix A = [cij ] ∈ Mn×n (K) is a lower-triangular matrix if and only if cij = 0K whenever i < j. Again, the set of all lower-triangular matrices is a subspace of the vector space Mn×n (K) over F and, indeed, an F -subalgebra. Note that a matrix A is upper triangular if and only if AT is lower triangular. A matrix A = [cij ] ∈ Mn×n (K) is symmetric if and only if A = AT . That is, A is symmetric if and only if cij = cji for all 1 ≤ i, j ≤ n. If B is any matrix in Mn×n (K) then B + B T is symmetric. If K is commutative and if C ∈ Mk×n (K) for any positive integers k and n, then CC T ∈ Mk×k (K) and C T C ∈ Mn×n (K) are symmetric. If n is a positive integer and F is a field, then v ∧ v is a symmetric matrix in Mn×n (F ) for all v ∈ F n . Diagonal matrices are clearly symmetric and the set of symmetric matrices in Mn×n (K) is closed under taking sums and scalar multiples, and so it is a subspace of the vector space Mn×n (K) over F. In the case K = F, the dimension of Mn×n (F ) equals n2 (n+1). However, the set of symmetric matrices is not closed under products. For     2 5 1 1 2 1 example, the matrices A =  5 2 0  and B =  2 0 0  in 1 0 1 1 0 3   13 4 5 M3×3 (R) are symmetric but AB =  9 10 5  is not. Nonetheless, 2 2 4 if A and B are a commuting pair of symmetric matrices then (AB)T = (BA)T = AT B T = AB, so AB is again symmetric. Similarly, a matrix A = [cij ] ∈ Mn×n (K) is skew symmetric if and only if A = −AT . The set of all skew-symmetric matrices in Mn×n (K) is again a subspace of Mn×n (K). Note that if F is a field having characteristic other than 2, then any matrix A ∈ Mn×n (K) can be written as the sum of a symmetric matrix and a skew-symmetric matrix, since A = 12 (A+AT )+ 12 (A−AT ). In one of the examples after Proposition 5.14, we saw that this representation is in fact unique. The Lie product of two skew-symmetric matrices is again skew-symmetric.


135

Example: Let n be a positive integer. A matrix A = [aij ] ∈ Mn×n (R) 1 is na Markov matrix if and only if aij ≥ 0 for all 1 ≤ i, j ≤ n and j=1 ahj = 1 for each 1 ≤ h ≤ n; it is a stochastic matrix if and only if both A and AT are Markov matrices. It is easy to show that the product of two Markov matrices is again a Markov matrix and the product of two stochastic matrices in Mn×n (R) is again a stochastic matrix. Markov matrices arise naturally in probability theory. In particular, if we have a system which, at each tick of a (discrete) clock, is in one of the distinct states s1 , . . . , sn and if, for each 1 ≤ i, j ≤ n, we denote by pij the probability that if the situation is in state i at a given time t then it will be in state j at time t + 1, the matrix [pij ] is a Markov matrix. As we have already pointed out, a matrix O = A ∈ Mn×n (F ) is not necessarily a unit. The units of the F -algebra of square matrices are known as nonsingular matrices; the other matrices are singular2 matrices. By what we have already noted, the product of nonsingular matrices is again nonsingular. Let V be a vector space over F of dimension n and let B be a basis of V. Then there exists an endomorphism α of V such that A = ΦBB (α). If A is a unit then there also exists an endomorphism β of V satisfying A−1 = ΦBB (β). This means that I = AA−1 = ΦBB (α)ΦBB (β) = ΦBB (αβ) and so αβ = σ 1 , and similarly βα = σ 1 . Therefore α ∈ Aut(V ) and β = α−1 . Example: Let F be a field and let n be a positive integer. If c ∈ F and v, w ∈ F n , then the matrix A = I + c(v ∧ w) is nonsingular if and only if the scalar 1 + c(v w) is nonzero. Indeed, direct computation shows that if 1 + c(v w) = 0, then A−1 = I + d(v ∧ w), where

1 Russian mathematician Andrei Markov made major contributions to probability theory at the beginning of the twentieth century.

2 These terms were first used by American mathematician Maxime Bˆ ocher in 1907. He was also the first to popularize the terms “linearly dependent” and “linearly independent”.

136

9. The algebra of square matrices −1

d = −c [1 + c(v w)] and if 1 + c(v w) = 0 then Av = v + c(v w)v is the 0-vector, and so A must be singular. Example: The multiplicative inverse of a “nice” nonsingular matrix may not be “nice”. Thus, if A is a nonsingular matrix all of the entries of which are nonnegative, it does not follow that all of the entries of A−1 are   1 1 1 nonnegative. For example, if we choose A =  1 2 1  then direct 1 1 2   3 −1 −1 1 0 . If A = [aij ] is the computation shows us that A−1 =  −1 −1 0 1 n × n tridiagonal matrix with aii = 2 for all 1 ≤ i ≤ n and aij = −1 whenever |i − j| = 1, then not only is A−1 not tridiagonal, but in fact no entries in A−1 equal 0, for any n > 1. Example: a prime positive integer. The complex number Let n 2πbe + i sin is called a primitive root of unity of degree cn = cos 2π n n n, since it easy to check that cnn = 1 but cin = 1 for all 0 < i < n. n−1 for all n. For each z ∈ C, let F (z) ∈ Mn×n (C) Therefore, c−1 n = cn be the matrix [aij ] defined by aij = z (i−1)(j−1) for all 1 ≤ i, j ≤ n. It is straightforward to show that the matrix F (cn ) is nonsingular and, n which indeed, F (cn )−1 = n1 F (c−1 n ). The endomorphism ϕn of C is represented with respect to the canonical basis by the matrix F (cn ) is called a discrete Fourier transform of Cn . This endomorphism is of great importance in applied mathematics. An algorithm, known as the fast Fourier transform (FFT), introduced by J. W. Colley and John W. Tukey3 in 1965, allows one to calculate ϕn (v) in an order of n log(n) arithmetic operations, rather than n2 , as one would anticipate. This facilitates the use of Fourier transforms in applications. A similar construction is also possible over finite fields, and especially over fields of the form GF (p). We will look at this example again in Chapter 15.

3 Joseph Fourier was a close friend of Napoleon and served for many years as permanent secretary of the Parisian Academy of Sciences. He worked primarily in applied mathematics, and developed many important tools in this area. John W. Tukey was a twentieth-century American statistician who developed many advanced mathematical tools in statistics.


137

A closely-related endomorphism, the discrete cosine transform is used in defining the JPEG algorithm for image compression. Example: The subset T of M2×2 (R) consisting of all matrices of the ! a b form is easily checked to be an R-subalgebra of M2×2 (R). −b a ! a b Moreover, the function γ : C → T given by γ : a + bi → is −b a an R-algebra isomorphism. Let K be an associative unital algebra over a field F having multiplicative identity e, and let n be a positive integer. Let E be the multiplicative identity of Mn×n (K) A matrix A = [cij ] ∈ Mn×n (K) is an elementary matrix if and only if it is of one of the following forms: (1) Ehk , the matrix formed from E by interchanging the hth and kth columns, where h = k; (2) Eh;c , the matrix formed from E by multiplying the hth column by 0K = c ∈ K; (3) Ehk;c , the matrix formed from E by adding c times the kth column to the hth column, where h = k, where c ∈ K. It is easy to verify that matrices of the form Ehk and Ehk;c are always −1 −1 = Ehk and Ekh;c = Ehk;−c . If c is a unit in nonsingular, with Ehk −1 K, then matrices of the form Eh;c are nonsingular, with Eh;c = Eh,c−1 . We note that the transpose of an elementary matrix is again an elementary T T = Ehk and Eh;c = Eh;c for all 1 ≤ h, k ≤ n and matrix. Indeed, Ehk T 0K = c ∈ K, while Ehk;c = Ekh;c for all 1 ≤ h = k ≤ n and all c ∈ K. As the name clearly implies, there is a connection between the elementary automorphisms which we defined previously and the elementary matrices. Indeed, if K = F and if B is the canonical basis of F n , then Ehk = Φ(εhk ), Eh;c = Φ(εh;c ), and Ehk;c = Φ(εhk;c ). Let us see what happens when one multiplies an arbitrary matrix in Mn×n (K) on the left by an elementary matrix: (1) If B ∈ Mn×n (K) then Ehk B is the matrix obtained from B by interchanging the hth and kth rows of B. Thus, for example, in M4×4 (Q) we look at the effect of E24 :      1 0 0 0 5 6 4 1 5 6 4 1  0 0 0 1  3 2 2 2   3 3 2 2        0 0 1 0  0 4 2 7  =  0 4 2 7 . 0 1 0 0 3 3 2 2 3 2 2 2 (2) If B ∈ Mn×n (K) then Eh;c B is the matrix obtained from B by multiplying the hth row of B by c. Thus, for example, in M4×4 (Q) we

138


look at the effect of  1 0 0  0 5 0   0 0 1 0 0 0

E2;5 :  0  0   0  1

5 3 0 3

6 2 4 3

4 2 2 2

  1 5  15 2  = 7   0 2 3

6 10 4 3

4 10 2 2

 1 10  . 7  2

(3) If B ∈ Mn×n (K) then Ehk;c B is the matrix obtained from B by adding c times the the hth row to the kth row. Thus, for example, in M4×4 (Q) we look at the effect of E13;2 :      1 0 0 0 5 6 4 1 5 6 4 1  0 1 0 0  3 2 2 2   3 2 2 2        2 0 1 0   0 4 2 7  =  10 16 10 9  . 0 0 0 1 3 3 2 2 3 3 2 2 (9.1) Proposition: If F is a field, if n is a positive integer, and if A, B, C, D ∈ Mn×n (F ) then: (1) When A and B are nonsingular, so is AB, with (AB)−1 = −1 −1 B A ; (2) When AB is nonsingular, both A and B are nonsingular; (3) When A and B are nonsingular, A−1 + B −1 = A−1 (B + A)B −1 ; (4) When I + AB is nonsingular, so is I + BA, and (I + BA)−1 = I − B(I + AB)−1 A; (5) (Guttman’s Theorem) If A is nonsingular and if v, w ∈ F n satisfy the condition that 1 + w A−1 v = 0, then the matrix −1 A + v ∧ w ∈ Mn×n (F ) is nonsingular and satisfies (A + v ∧ w) = −1 A−1 [v ∧ w]A−1 . A−1 − 1 + w A−1 v (6) (Sherman-Morrison-Woodbury Theorem4 ) When the matrices C, D, D−1 + AC −1 B and C + BDA are nonsingular, then (C + BDA)−1 = C −1 − C −1 B(D−1 + AC −1 B)−1 AC −1 .

4

Louis Guttman was a 20th-century American/Israeli statistician and sociologist, who developed many advanced mathematical tools for use in statistics. Jack Sherman, Winifred J. Morrison, and Max Woodbury were 20th-century American statisticians.


139

Proof: (1) This is a special case of a general remark about units in associative F -algebras, which we have already noted. (2) Let V a vector space of dimension n over F, and let D be a basis of V. Then there exist endomorphisms α and β of V satisfying A = ΦDD (α) and B = ΦDD (β), and so AB = ΦDD (αβ). Since AB is nonsingular, we know that αβ ∈ Aut(V ). Then there exists an automorphism γ of V satisfying γ(αβ) = σ 1 = (αβ)γ. Then (γα)β = σ 1 = α(βγ) and so, by Proposition 7.4, we know that both α and β are automorphisms of V and hence both A and B are nonsingular. (3) This is an immediate consequence of the fact that A(A−1 +B −1 )B = B + A. (4) We note that ) ( (I + BA) I − B(I + AB)−1 A = I + BA − (B + BAB)(I + AB)−1 A =

I + BA − B(I + AB)(I + AB)−1 A

=

I + BA − BA = I.

(5) A simple calculation shows us that if x, y ∈ F n satisfy the condition that c = 1 + y x is nonzero, then I − c−1 [x ∧ y] (I + [x ∧ y]) = I + x ∧ y − c−1 [x ∧ y] − c−1 [x ∧ y]2 = −1

and so (I + [x ∧ y]) A−1 v, then −1

(A + v ∧ w)

= = =

I + x ∧ y − c−1 c[x ∧ y] = I

= I − c−1 [x ∧ y] . Therefore, if we set d = 1 + w

( )−1 −1 −1 A I + A−1 [v ∧ w] = I + A−1 [v ∧ w] A −1 ( ) −1 −1 A [v ∧ w] A I −d −1 −1 −1 A [v ∧ w]A−1 A −d

as required. (6) First note that I + C −1 BDA = C −1 (C + BDA) and so, by (1), this matrix too is nonsingular. By (4), (I + C −1 BDA)−1 = I − C −1 B(I + (DAC −1 B)DA and so (C + BDA)−1

(

)−1 C(I + C −1 BDA)

=

(

=

) I − C −1 B(I + DAC −1 B)−1 DA C −1 ( )−1 C −1 − C −1 B D−1 (I + DAC −1 B) AC −1

=

C −1 − C −1 B(D−1 + AC −1 B)−1 AC −1 .

=

as required.

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Guttman’s Theorem is important in the following context: assume we have calculated A−1 for some square matrix A and now we have to calculate B −1 , where B differs from A in only one entry. With the help of this result, we can make use of our knowledge of A−1 to calculate B −1 with relative ease and speed. The Sherman-Morrison-Woodbury Theorem has similar uses. In particular, we note from Proposition 9.1 that, if A, B ∈ Mn×n (F ), then AB is nonsingular if and only if BA is nonsingular. We should also note that, if A, B ∈ Mn×n (F ), then B T AT = (AB)T and so, if A is a nonsingular matrix and B = A−1 then AB = I and so B T AT = I T = I and so AT is also nonsingular. Moreover, this shows that (AT )−1 = (A−1 )T for every nonsingular matrix A ∈ Mn×n (F ). (9.2) Proposition: Let F be a field, let n be a positive integer, and let A, B ∈ Mn×n (F ), where A is nonsingular. Then there exist unique matrices C and D in Mn×n (F ) satisfying CA = B = AD. Proof: Define C = BA−1 and D = A−1 B. Then surely CA = B = AD. If C and D are matrices satisfying C A = B = AD then C = (C A)A−1 = BA−1 = C and D = A−1 (AD ) = A−1 B = D, and so we have uniqueness. Example: The matrices C and D in Proposition 9.2 need not be the ! 1 3 same. For example, if A, B ∈ M2×2 (R) are defined by A = 0 1 ! ! ! 1 −3 1 −3 1 0 , C = and and B = then A−1 = 0 1 3 −8 3 1 ! −8 −3 D= . 3 1 (9.3) Proposition: Let F be a field, let n be a positive integer, and let A = [aij ] ∈ Mn×n (F ). Then the following conditions are equivalent: (1) A is nonsingular; (2) The columns of A are distinct and the set of these columns is a linearly-independent subset of F n ; (3) The rows of A are distinct and the set of these rows is a linearly-independent subset of M1×n (F ). Proof: (1) ⇔ (2): Denote the columns of A by y1 , . . . , yn . Let V = F n and let B = {v1 , . . . , vn } be the canonical basis of V. If two columns of A are equal or if the set of columns is linearly dependent, there exist scalars


141



   c1 0     n c1 , . . . , cn , not all equal to 0, such that A  ...  = i=1 ci yi =  ...  . 0 cn       c1 0 0  ..   ..  −1  ..  But if (1) holds, then  .  = A  .  =  .  , which is a cn

0

0

contradiction. Therefore (2) holds. Conversely, assume (2) holds. Then the endomorphism α of V given by v → Av is a monic and so an automorphism of V. But A = ΦBB (α), and so, as we have seen, A is nonsingular. (1) ⇔ (3): This follows directly from the equivalence of (1) and (2), given the fact that a matrix A is nonsingular if and only if AT is nonsingular. Example: Let F be a field and let n > 1 be an integer. If v, w ∈ F n , then the columns of v ∧w ∈ Mn×n (F ) are linearly dependent and so v ∧w is always singular. Example: If F is a field and if U = [uij ] ∈ Mn×n (F ) is an uppertriangular matrix satisfying the condition that uii = 0 for all 1 ≤ i ≤ n then, by Proposition 9.3, it is clear that U is nonsingular. We claim that, moreover, U −1 is again upper triangular. Let us prove this contention by induction on n. It is clearly true for n = 1. Assume therefore that n > 1 and that we have already shown that the inverse of any upper-triangular ! A y , matrix in M(n−1)×(n−1) (F ) is upper-triangular. Write U = z unn  T 0  ..  n−1 where A ∈ M(n−1)×(n−1) (F ), y ∈ F , . and z =  .  . Assume that U −1 =

B wT

x b

!

0 , where B ∈ M(n−1)×(n−1) (F ) and w, x ∈ F n−1 .

Then AB + y ∧ w = I, Ax + by = z T , unn wT = z, and unn b = 1, so T we must have b = u−1 nn = 0 and w = z. Therefore y ∧ w = O and so −1 B = A . By hypothesis, B is upper triangular and so U −1 is again upper triangular. A similar argument holds for lower-triangular matrices. (9.4) Proposition: Let F be a field and let n be a positive integer. A matrix in Mn×n (F ) is nonsingular if and only if it is a product of elementary matrices.

142


Proof: Since each of the elementary matrices is nonsingular, we know that any product of elementary matrices is also nonsingular. Conversely, let A = [aij ] be a nonsingular matrix in Mn×n (F ) and let B = [bij ] be A−1 . Then B is also nonsingular and so, by Proposition 9.3, the columns of B are distinct and the set of columns is linearly independent in F n . In particular, there exists a nonzero entry bh1 in the first column of B. Multiply B on the left by Eh1 to get a new matrix in which the (1, 1)entry nonzero. Now multiply it on the left by E1;c , where c = b−1 h1 , in   1 * ... *  * * ... *    order to get a matrix of the form  . . ..  . Now let 1 < t ≤ n, . .  . . .  * * ... * and let d(t) be the additive inverse of the (t, 1)-entry of the matrix. Multiplying the matrix on the left by Et1;d(t) , we will get a matrix with 0 in the (t, 1)-entry and so, after this for each such t, we see that a matrix B = C1 B, where C1 is a product of elementary matrices, and which is   1 * ... *  0 * ... *    of the form  . . ..  . This matrix is still nonsingular, since it  .. .. .  0 * ... * is a product of two nonsingular matrices, and so its columns are distinct and form a linearly-independent subset of F n . Therefore there exists a nonzero entry bh2 in the second column, with h > 1. Repeating the above procedure, we can find a matrix C2 which is a product of elementary   1 0 * ... *  0 1 * ... *      matrices and such that C2 C1 B is of the form  0 0 * . . . *  .  .. .. .. ..   . . . .  0 0 * ... * Continuing in this manner, we obtain matrices C1 , . . . , Cn , each of them a product of elementary matrices, such that Cn · . . . · C1 B = I. Therefore Cn · . . . · C1 = B −1 = A, as we wanted to show.

Example: Let F be a field and let n be a positive integer. Every permutation π of the set {1, . . . , n} defines a matrix Aπ = [aij ] ∈ Mn×n (F ) by setting aij = 1 if j = π(i) and aij = 0 otherwise, called the permutation matrix defined by π. This matrix is clearly a result of multiplying I by a number of elementary matrices of the form Ehk , and so is nonsingular.


143

Proposition 9.4 allows us to construct an algorithm for computing A−1 when A is a(nonsingular matrix in Mn×n (F ). First of all, we construct ) I A ∈ Mn×2n (F ) and on this matrix we perform a the matrix series of elementary operations, namely operations which are the result of multiplying it on the left by elementary matrices, which bring the righthand block into the form I. Then the left-hand block is A−1 . To calculate A−1 by this method, we use n3 −2n2 +n additions and n3 multiplications. 

1 2 Example: Consider the matrix A =  2 3 0 1  1 0 0 1 2 fore we begin with the matrix  0 1 0 2 3 0 0 1 0 1   1 0 0 1 2 3 (1) Get  −2 1 0 0 −1 −6  after 0 0 1 0 1 2 by −2 and adding it to the second row; 

1 0 0 1 (2) Get  −2 1 0 0 −2 1 1 0 the third row; 

1 (3) Get  2 0.5

0 −1 −0.25

 3 0  ∈ M3×3 (Q). There2  3 0  ∈ M3×6 (Q). Then: 2 multiplying the first row

 2 3 −1 −6  after adding the second row to 0 −4

0 0 −0.25

 1 2 3 0 1 6  after multiplying the second 0 0 1

row by −1 and then multiplying the third row by −0.25; 

1 0 0.5 (4) Get  −1 0.5 −0.25

0 1.5 −0.25

 1 2 3 0 1 0  after multiply the third 0 0 1

row by −6 and adding it to the second row;  (5)

Get

 −0.5 0.75 0.75 1 2 0  −1 0.5 1.5 0 1 0  0.5 −0.25 −0.25 0 0 1

after multiplying the

third row by −3 and adding it to the first row; 

1.5 −0.25 −2.25 0.5 1.5 (6) Finally, get  −1 0.5 −0.25 −0.25

 1 0 0 0 1 0  after multiplying 0 0 1

the second row by −2 and adding it to the first row.

144


Therefore we see that A−1

  6 −1 −9 1 −4 2 6 . = 4 2 −1 −1

Example: When one uses computer to compute matrix inverses, one must always be aware of hardware limitations. For example, one can show ! 888445 887112 that Nievergelt’s matrix A = ∈ M2×2 (Q) is non887112 885871 ! 1 c c (which singular, while the matrix B = A− , where c = c c 3548450 is approximately 2.81813186039 × 10−7 ) is not. Nonetheless, a computer or calculator capable of only 12-digit accuracy cannot differentiate between the two. Example: For each positive integer n, let Hn ∈ Mn×n (Q) be the 1 . This matrix is called the n × n matrix [aij ], in which aij = i+j−1 5 Hilbert matrix . The Hilbert matrices are all nonsingular but, while their entries all lie between 0 and 1, the entries in their inverses are very large. For example, H6−1 equals   36 −630 3360 −7560 7560 −2772  −630 14700 −88200 211680 −220500 83160     3360 −88200 564480 −1411200 1512000 −582120     −7560 211680 −1411200 3628800 −3969000 1552320     7560 −220500 1512000 −3969000 4410000 −1746360  −2772 83160 −582120 1552320 −1746360 698544 Therefore these matrices are often used as benchmarks to judge the efficiency and accuracy of computer programs to calculate matrix inverses. In particular if the computer we are using has only 7-digit accuracy, it is reasonable to assume that we will have a 100% error in computing H6−1 . It is sometimes possible to use a representation of a nonsingular matrix A in block form in order to calculate A−1 . Indeed, suppose that A ∈

5 German David Hilbert was one of the foremost mathematicians in the world at the beginning of the 20th century. He and his students were among the first to study infinite-dimensional vector spaces.


Mn×n (F ) is a matrix which can be written in block form

A11 A21

145

A12 A22

! ,

where A11 ∈! Mk×k (F ). In order to find A−1 , we must find a matrix B11 B12 , where B11 ∈ Mk×k (F ), such that B21 B22 A11 B11 + A12 B21

=

I

A11 B12 + A12 B22

= =

O O

=

I

A21 B11 + A22 B21 A21 B12 + A22 B22

and if we know that the matrix A11 is itself nonsingular, then from the first equation we immediately see that B11 = A−1 11 (I − A12 B21 ). If we substitute this in the third equation, we obtain )−1 ( B21 = − A22 − A21 A−1 A21 A−1 11 A12 11 , under the assumption, of course, that the matrix C = A22 −A21 A−1 11 A12 is −1 A and nonsingular. In the same manner, we also obtain B12 = −A−1 11 12 C −1 B22 = A22 (I − A21 B12 ) if the matrix A22 is nonsingular. Thus we see that a sufficient condition for A to be nonsingular is that we can partition it as above in such a manner that A11 , A22 , and A22 − A21 A−1 11 A12 are all nonsingular. Let F be a field and let k and n be positive integers. Two matrices B, C ∈ Mk×n (F ) are equivalent if and only if there exist nonsingular matrices P ∈ Mk×k (F ) and Q ∈ Mn×n (F ) such that P BQ = C. This is, indeed, an equivalence relation on Mk×n (F ) since: (1) IBI = B for each such matrix B, showing that B is equivalent to itself; (2) If P BQ = C then P −1 CQ−1 = B; (3) If P BQ = C and P CQ = D then (P P )B(QQ ) = D, where we note that both P P and QQ are again nonsingular. Similarly, we say that B and C are row equivalent if and only if there exists a nonsingular matrix P ∈ Mk×k (F ) satisfying P B = C, and we say that B and C are column equivalent if and only if there exists a nonsingular matrix Q ∈ Mn×n (F ) satisfying BQ = C. Both of these relations are also equivalence relations on Mk×n (F ), and it is clear that if B and C are row equivalent then they are equivalent (take Q = I) and if they are column equivalent then they are equivalent (take P = I). Equivalence of matrices is a very strong concept. Indeed, it is easy to show that any matrix B ∈ Mk×n (F ) is equivalent to one which is in block

146


form

I O

O O

! . Therefore, it is more useful to consider row equivalence

of matrices as our basic tool. Now let V be a vector space of dimension n over a field F and choose bases B = {v1 , . . . , vn } and D = {w1 , . . . , wn } of V. For each 1 ≤ j ≤ n there exist elements q1j , . . . , qnj of F satisfying n 9.3, wj = i=1 qij vi . By Proposition n we know that the matrix Q = [qij ] n is nonsingular. If v = i=1 ai vi = j=1 bj wj is an element of V, then we n n n n n see that v = j=1 bj wj = j=1 bj ( i=1 qij vi ) = i=1 j=1 qij bj vi n and so we must have ai = j=1 qij bj for all 1 ≤ i ≤ n. Thus we see     a1 b1     that  ...  = Q  ...  . The matrix Q is called the change-of-basis an

bn

matrix from D to B. Example: Let F be a field, let n be a positive integer, and let V be the subspace of the vector space F [X] made up of all polynomials of degree at most n − 1. Then dim(V ) = n, and it has a canonical basis B = {1, X, . . . , X n−1 }. Let c1 , . . . , cn be distinct scalars, and for each 1 ≤ i ≤ n, consider the polynomial 1 (X − cj ) ∈ V. pi (X) = ci − cj j=i

This polynomial is called the ith Lagrange interpolation polynomial, and we will return to these polynomials below in another context. It is clear that

1 if i = j . pi (cj ) = 0 otherwise Thus, for example, if n = 4 and if we choose c1 = 1, c2 = 3, c3 = 5, and c4 = 7, we obtain 35 1 3 5 71 X + X2 − X + 48 16 48 16 35 1 3 13 2 47 X − X + X− 16 16 16 16 21 −1 3 11 2 31 X + X − X+ 16 16 16 16 5 1 3 3 2 23 X − X + X− . 48 16 48 16

p1 (X)

= −

p2 (X)

=

p3 (X)

=

p4 (X)

=

Returning to the general case, we see that the set D = {p1 (X), . . . , pn (X)} of Lagrange interpolation polynomials is linearly independent since, if we


147

n

ah = i=1 ai pi (X) = 0, then for each 1 ≤ h ≤ n we have a p (c ) = 0. Therefore D is also a basis of V. If q(X) is an i i h i=1 arbitrarypolynomial in V then there exist scalars a1 , . . . , an satisfying n q(X) = i=1 ai pi (X); Again, this implies that ai = q(ci ) for all i. In n particular, if q(X) = X k we see that X k = i=1 cki pi (X). Therefore   1 c1 . . . cn1  1 c2 . . . cn2    the change of basis matrix from D to B is  . .. ..  . A .  . . .  have n

1

cn

...

cnn

matrix of this form is called a Vandermonde matrix, and such matrices are always nonsingular6 . Lagrange interpolation allows us to represent a polynomial p(X) of degree less than n in a computer not by its list of coefficients but rather by a list of its values p(a1 ), . . . , p(an ) at n preselected elements of F. Such representations can be used to obtain algorithms for rapid multiplication of polynomials, especially in the case the field F is finite. Let us now return to the matter of change of basis, and now let us assume that we have a linear transformation α : V → Y, where V is a vector space of dimension n over a field F and Y is a vector space of dimension k over F. We have bases B = {v1 , . . . , vn } and D = {w1 , . . . , wn } of V. Choose a basis E = {y1 , . . . , yk } of Y . Then ΦBE (α) is a matrix C = [cij ]. If Q = [qij ] is the change of basis n matrix from nD to B then ) = α ( q v ) = for each 1≤ j ≤ n we have α(w j h=1 hj h h=1 qhj α(vh ) = k k n n = i=1 ( h=1 cih qhj ) yi and so ΦDE (α) = CQ, h=1 qhj i=1 cih yi showing that ΦDE (α) and C are column equivalent. In the same manner, if we have another basis G = {z1 , . . . , zk } of Y and if P = [pij ] is k the change of basis matrix from E to G, then zj = i=1 pij yi for all 1 ≤ j ≤ k. If ΦBG (α) is the matrix C = [cij ], then for all k k k = 1 ≤ j ≤ n we have α(vj ) = h=1 ehj zh = h=1 ehj i=1 pih yi

6

Joseph-Louis Lagrange was one of the applied mathematicians who surrounded Napoleon, and his book on analytical mechanics is considered a mathematical classic. Alexandre-Th´ eophile Vandermonde was an 18th century French chemist and mathematician who studied determinants of matrices. Vandermonde matrices do not appear in his work, and it is not clear why they are named after him.

148

k i=1


k h=1 pih ehj −1

yi and this equals

k

i=1 cij yi

and so C = P C and

so C = P C. Thus ΦBG (α) and C are row equivalent. If we put both of these results together, we see that ΦDG (α) = P −1 ΦBE (α)Q, and so ΦDG (α) and ΦBE (α) are equivalent.

Example: Let α : R3 → R2 be the linear transformation given by α :        ! a 0 0   1  b  → a + b . Choose bases B =  0  ,  1  ,  −1  and b+c   c 0 1 0      

! !1 0   1 1 0 , D =  0  ,  0  ,  1  of R3 and bases E = 0 −1   0 1 −1

! !! 1 1 1 1 −1 and G = , of R2 . Then ΦBE (α) = 1 −1 0 −2 1 since 



 1 α  0  = 0   0 α  1  = 1   0 α  −1  = 0

and, similarly,

ΦDG (α) =

1 2

1 0 1 2

!

1 0 1 1 1 0

!

= (−1)

1 1 !

−2

0 −1

1 0

!

!

!

0 −1

+1

! ,

1 = 2

1 1

=1

1 1

1 = 2

1 1

!

!

+0

0 −1

!

!

2 0



 1 α  0  = 0   1 α  0  = 1   0 α  1  = −1

=1

1 0

!

−1 −1

1 1

=1

1 0

!

1 + 2

! +0 !

1 + 2

1 −1 1 −1 1 −1

!

!

!

!


149



       1 1 0 0 Further, we also see that  0  = 1  0  + 0  1  + 0  −1  , 0 0 1 0             1 1 0 0 0 1  0  = 1  0  + 1  1  + 1  −1  , and  1  = 0  0  − 1 0 1 0 −1 0       0 0 1 1 0 1  1  − 2  −1  so Q =  0 1 −1  . 1 0 ! ! 0 1 −2 ! ! ! 1 1 0 1 1 Moreover, = 1 −1 and = 1 + 1 0 −1 −1 0 ! ! ! 1 1 −1 0 1 1 −1 . Note that = 1 so P = and P 1 −1 −1 1 2 1 −1 P ΦBE (α)Q = ΦDG (α).

Example: We will now see an application of linear algebra to calculus. Let V be the vector space over R consisting of all infinitely-differentiable functions f ∈ RR , and let δ ∈ End(V ) be the differentiation endomorphism. (1) If a and b are given real numbers, not both equal to 0, then the functions f0 : x → eax sin(bx) and f1 : x → eax cos(bx) belong to V and the subspace W = R{f0 , f1 } of V is invariant under δ. The restriction of δ to W can be represented with respect to the basis ! a −b . It is easy to {f0 , f1 } of W by the nonsingular matrix A = b a ! a b 1 . Therefore check that A−1 = a2 +b 2 −b a 6 f0 (t)dt

=

f1 (t)dt

=

6

1 [af0 − bf1 ] and a2 + b2 1 [bf0 + af1 ]. δ −1 (f1 ) = a2 + b2 δ −1 (f0 ) =

(2) The functions g0 : x → x2 ex , g1 : x → xex , and g2 : x → ex all belong to V and the subspace Y = R{g0 , g1 , g2 } of V is invariant under δ. The restriction of δ to Y can be represented with respect to the basis   1 0 0 {g0 , g1 , g2 } of Y by the nonsingular matrix B =  2 1 0  . Since 0 1 1

150




B −1

1 =  −2 2

 0 0 1 0  , we see that −1 1 6 g0 (t)dt = δ −1 (g0 ) = g0 − 2g1 + 2g2 , 6 g1 (t)dt = δ −1 (g1 ) = g1 − g2 , and 6 g2 (t)dt = δ −1 (g2 ) = g2 .

Let us turn to problems connected with the implementation of this theory. Let F be a field and let n be a positive integer. Let A = [aij ] and B = [bij ] belong to Mn×n (F ) and let C = AB. In order to calculate each one of the n2 entries in C, we need n multiplications and n − 1 additions/subtractions, and so to calculate C we need n3 multiplications and n3 − 2n2 + n additions/subtractions. Putting this in another way, the total number of operations needed to calculate AB from the definition is on the order of nc , where c = 3. If n is very large, this can entail considerable computational overhead and leaves room for the introduction of considerable error due to roundoff and truncation in the course of the calculation. It is therefore very important to find a more sophisticated method of matrix multiplication, if possible. One such method is the Strassen-Winograd algorithm7 . To illustrate the Strassen-Winograd algorithm, let us first begin with the special case n = 2. First, calculate p0 = (a11 + a12 )(b11 + b12 ) p1 = (a11 + a22 )b11 p3 = (a21 − a11 )(b11 + b12 ) p4 = (a11 + a12 )b22 p6 = (a12 − a22 )(b21 + b22 ) and then note that C =

p 0 + p5 − p4 + p6 p1 + p5

p2 = a11 (b12 − b22 ) p5 = a22 (b21 − b11 )

p2 + p4 p0 − p1 + p2 + p3

! . In

this calculation, we used 7 multiplications and 18 additions/subtractions

7

Variants of this algorithm were discovered by the contemporary German mathematician Volker Strassen and the contemporary Israeli mathematician Shmuel Winograd, who later served as director of mathematical research at IBM.


151

(Winograd’s variant of this algorithm uses only 15 additions/subtractions, but these are more interdependent, and so the algorithm is less amenable to implementation on parallel computers) instead of 8 multiplications and 4 additions/subtractions. In the early days of computers, when multiplication was several orders of magnitude slower than addition, this in itself was a great accomplishment. If n = 4, we write our matrices in ! ! B11 B12 A11 A12 and B = , where each block form: A = A21 A22 B21 B22 block is a 2 × 2 matrix. We now calculate 2 × 2 matrices P0 , . . . , P6 and then construct C = AB as above. To do this, we need 49 multiplications and 198 additions/subtractions, as opposed to 64 multiplications and 46 additions/subtractions if one goes according to the definition. We continue recursively. If n = 2h , then the number of multiplications needed is M (h) = 7h and the number of additions/subtractions needed is A(h) = 6(7h − 4h ) and so M (h) + A(h) < 7h+1 . (If n is not a power of 2, we can add rows and columns of 0’s in order to enlarge it to the desired size.) Thus, we see that the number of arithmetic operations needed to calculate AB is on the order of nc , where c ≤ log2 7 = 2.807 . . . and so, for large n, we have a definite advantage over multiplication following from the definition. Using even more sophisticated techniques, it is possible to reduce the number of arithmetic operations to the order of nc , where c ≤ 2.376 . . . , as was done by Winograd and Coppersmith in 1986. The size of matrices for which the Strassen-Winograd algorithm is significantly faster than the regular method depends, of course, on the particular hardware on which it is being used. The Strassen-Winograd algorithm can also be modified to multiplication of matrices which are not necessarily square.

Unfortunately, the Strassen-Winograd algorithm is no less susceptible to roundoff and truncation errors than the regular algorithm. On a computer with seven-digit accuracy, the product 

 211 2 3 4 50    60 1 2 3 4    0.001 0.032 0.043 0.044   23 311 0.0032 1233 0.0324 33 

10871  371 equals   4.411 43910.3

67.834 0.634 0.0043 138.977

0.7293 0.2463 0.0033 37.7061

0.32 0.023 0.032 0.043

0.0023 0.033 0.03 0.022

 421 982   623  44

 92840  4430  using the ordinary me 60.57 899094.0

thod of matrix multiplication, whereas, using the Strassen-Winograd algo-

152




10871  370.9 rithm, we obtain   4.411 43910.3

68.54 1.0 0.0043 139.047

 0.6294 92840 0.2463 4430.18   . This prob 0 62.0 37.7 899095.0

lem can be overcome to some extent by stopping the recursion in the Strassen-Winograd algorithm early, and doing the bottom-level matrix multiplication using the ordinary method. Another disadvantage of this algorithm is that it requires a much larger amount of scratch memory space to perform its calculations. There are other tricks that can be used to reduce the computations necessarily in matrix multiplication. For example, if n is a positive integer and if A, B, C, D ∈ Mn×n (R), then the matrix product (A + iB)(C + iD) in Mn×n (C) can be calculated using only three matrix multiplications in Mn×n (R), rather than the expected four, by noting that (A + iB)(C + iD) = AC − BD + i [(A + B)(C + D) − AC − BD] . Again, we keep in mind that real and complex numbers are represented in a computer by approximations having a limited degree of accuracy. The longer calculations become, the error due to roundoff and truncation increases and limits the correctness of the calculations. It is possible to reduce the effect of roundoff and truncation errors as much as possible. Let us recall how our algorithm( for inverting a matrix A worked: ) I A = [bij ]; (1) We formed the matrix (2) We interchanged the first row which one of the rows below it, if necessary, such that b1,n+1 = 0; we then multiplied this row by b−1 1,n+1 so that this element is now equal to 1, and we subtracted multiples of this row from the rows below it, in order to make bi,n+1 equal to 0 for all 1 < i ≤ n. (3) We now go iterate this process for the elements bh,n+h , where h = 2, 3, . . . and so forth. If we cannot do it, i.e. if there exists an h such that bi,n+h for all h ≤ i ≤ n, the matrix A is nonsingular. Otherwise, ( −1at the) end of the process, we have brought the matrix to the I . A form The elements bh,n+h are called pivots of the algorithm. If we are working over the real or complex numbers, we can minimize roundoff and truncation errors – to some extent – by making sure that each time we interchange rows we choose to bring into the pivot position a nonzero number having maximal absolute value. This strategy is known as partial pivoting. We could do better by also interchanging columns in order to bring into the pivot position bh,n+h the element bij (h ≤ i, j ≤ n) having maximal absolute value. This strategy is known as full pivoting and it


153

requires a certain amount of computational overhead on the side so that the columns can be returned to their proper positions at the end of the algorithm. Although there are matrices so pathological that full pivoting rather than partial pivoting is needed in order to invert them, most experts believe that the effort is not worth the effort and the computational overhead and that for such matrices it is best to use other methods altogether. Several variants of pivoting strategies for matrices having specific structures have, however, been developed and are in use. Indeed, let us now consider another method. It is clearly easier to invert a nonsingular upper-triangular or lower-triangular matrix – namely a matrix in one of these forms all of the diagonal elements of which are nonzero. Therefore our job would be much easier if we could write A in the form LU, where L is lower triangular and U is upper triangular8 , for then A−1 = U −1 L−1 . This is not always possible. For example, one can see ! 0 1 that there is no way of writing the matrix ∈ M2×2 (R) in this 1 0 form. However, it is always possible to write A in the form LU when A equals a product of elementary matrices of the form Ei;c and Eij;c only. How can this be done? Assume that A = [aij ], U = [uij ], and L = [vij ] and that A = LU, where U is upper-triangular L is lower-triangular. and n Then for each 1 ≤ i, j ≤ n we have aij = h=1 vih uhj . In each of L and U there are only 12 (n2 + n) entries which can be nonzero and so our problem is one of solving n2 nonlinear equations in n2 + n unknowns. This means that we can allow ourself to choose the value of n of these variables arbitrarily, and we will do so by insisting that vii = 1 for all 1 ≤ i ≤ n. Now we have a system of n2 + n nonlinear equations in n2 + n unknowns, which can be solved by a method known as Crout’s algorithm9 : (1) First set vii = 1 for all 1 ≤ i ≤ n; (2) For all 2 ≤ j ≤ n and all 1 ≤ i ≤ j, first calculate uij = aij − j−1 i−1 1 h=1 vih uhj and then vij = ujj aij − h=1 vih uhj for all j < i ≤ n.

8 The LU method was devised by British mathematician Alan Turing, who is better known as the founder of automata theory and one of the fathers of the electronic computer. It appears implicitly in the work of Jacobi on bilinear forms. 9 This algorithm was devised by 20th-century American mathematician Prescott Crout.

154


We note that if A is a nonsingular matrix which can be written in the form LU , where L = [vij ] is a lower-triangular matrix satisfying vii = 1 for all 1 ≤ i ≤ n and U = [uij ] is upper-triangular, then this factorization must be unique. Indeed, assume that L1 U1 = L2 U2 where the Lh are lower triangular matrices with 1’s on the diagonal, and the −1 Uh are nonsingular upper-triangular matrices. Then L−1 2 L1 = U2 U1 . Since the product of lower-triangular matrices is lower triangular and the product of upper-triangular matrices is upper triangular, this matrix must be a diagonal matrix. But then L−1 2 L1 = I and so L1 = L2 and that implies that U1 = U2 , proving uniqueness. Example: The above uniqueness result is no A is singular. For example,     1 −1 2 1 0 0  −1 1 −1  =  −1 1 0   2 −2 4 2 b 1

longer true if the matrix

1 0 0

−1 0 0

 2 1  −b

for any scalar b ∈ R. As was previously remarked, not all nonsingular matrices can be written in the form LU, but one can show that for any nonsingular matrix A there exists a permutation matrix P such that A = P LU, where L is lower triangular and U is upper triangular. 

 0 1 1 −3  −2 4 1 4   = P LU, where Example: It is easy to verify that   0 0 0 1  3 1 1 0     0 1 0 0 1 0 0 0  1 0 0 0   0 1 0 0     P =  0 0 0 1  is a permutation matrix, L =  − 3 7 1 0  2 0 0 0 1 0 0 1 0   −2 4 1 4  0 1 1 −3   is lower triangular, and U =   0 0 − 9 27  is upper triangular. 2 0 0 0 1

Exercises




1 Exercise 390 Let F = GF (5). Calculate  2 1 in M3×3 (F ).

3 1 2

 1 1 1  4 3 1

155

2 3 4

 2 2  2

Exercise 391 Does there exist a real number b such that the matrices     b −1 −1 0 1 0 −1 0  0 1  b 0 −1  0 −1    and B =  −1 A= b  1 0 −1  1 −1  0  0 2 b 0 1 0 −1 0 1 −1 2 are a commuting pair in M4×4 (R)? Exercise 392 Let F = GF (7) and let K be the subalgebra of M2×2 (F ) ! a b consisting of all matrices of the form , for a, b ∈ F. Show −b a that K is a field. Is it a field if F = GF (5)? ! 1 1 Exercise 393 Let A = ∈ M2×2 (R). Find the set of all matri0 1 ces B ∈ Mn×n (R) satisfying BA = AB. ! 1 i Exercise 394 Let A = ∈ M2×2 (C). Find a complex number −i 1 c satisfying (cA)2 = A.   0 1 0 Exercise 395 Let A =  0 0 1  ∈ M3×3 (R). Find a positive integer 1 0 0 k −1 k satisfying A = A . Exercise 396 Let  0 isfying A2 =  0 0

F be a field. Find all matrices A ∈ M3×3 (F ) sat 0 1 0 0 . . 0 0

Exercise 397 Show that there are infinitely-many pairs (a, b) of real numbers satisfying the condition       a 0 0 1 0 1 1 0 1 a 0 0  0 1 0  0 1 0  =  0 1 0  0 1 0 . 0 0 b 1 0 1 1 0 1 0 0 b Exercise 398 Does there exist a   0 1 0 0  0 0 1  0 1 0 0 1

positive integer k satisfying  k  0 0 1 0 1 1 0  =  1 0 0 ? 0 1 0 0 0

156


Exercise 399 Let F = GF (3). Show that there exist at least 27 distinct matrices A in M3×3 (F ) satisfying A3 = I. Exercise 400 Let n be a positive integer and let F be a field of characteristic 0. Show that AB − BA = I for all A, B ∈ Mn×n (F ) (in other words, that I is not the product of any two elements of the Lie algebra Mn×n (F )− ). Exercise 401 If F = GF (2), find the set of all pairs (A, B) of matrices in M2×2 (F ) satisfying AB − BA = I. Exercise 402 For a field F, find

.

/ A ∈ M2×2 (F ) | A2 = O .

Exercise 403 Find a matrix A ∈ M3×3 (R) satisfying 

1 A 2 1

   1 −1 1 −1 3 1 0 = 4 3 2 . −1 1 1 −2 5 

 a 1 0 Exercise 404 Show that if A =  0 a 1  ∈ M3×3 (R) then for each 0 0 a   an nan−1 n(n−1) an−2 2 . n > 1 we have An =  0 an nan−1 n 0 0 a Exercise 405 Let (K, •) be an associative unital algebra over a field F and let S be the subset of M3×3 (K) consisting of all matrices of the   v11 0K v13 form  0K v22 0K  . Is S an F -subalgebra of M3×3 (K)? v31 0K v33 Exercise 406 Let n be a positive integer and let F be a field. A matrix   a1 a2 . . . an  an a1 . . . an−1   is called a circulant in Mn×n (F ) of the form    ... a1 a2 a3 . . . matrix. Show that the set of all circulant matrices in Mn×n (F ) is an F -subalgebra of Mn×n (F ). Exercise 407 Let n be a positive integer and let F be a field. If A ∈ Mn×n (F ) is a nonsingular circulant matrix, is A−1 necessarily a circulant matrix?


157

Exercise 408 Let K be the subset of M2×2 (Q) consisting of all matrices ! a b of the form , where a, b ∈ Q. Show that K is a Q-subalgebra 2b a of M2×2 (Q) which is, in fact, a field. Exercise 409 Find a matrix A ∈ M2×2 (R) satisfying A = 2

1 0

3 1

! .

A ∈ M3×3 (R) satisfying  1 1 2 2  = O. 1 1 ! b ∈ M2×2 (R) be a matrix satisfying d

Exercise 410 Find all matrices  1 A 2 0 Exercise 411 Let A =

a c

A2 = A. Show that a + d ∈ {0, 1, 2}. !n 1 1 = Exercise 412 Show that 1 1

2n−1 2n−1

Exercise 413 Let F be a field and let A = An for all n ≥ 1.

! 2n−1 for all n ≥ 1. 2n−1 ! 0 b ∈ M2×2 (F ). Find c 0

Exercise 414 Find matrices A, B ∈ M2×2 (Q) for which (A − B)(A + B) = A2 − B 2 .  1 0 Exercise 415 Let F be a field and let A =  1 0 0 1

 0 1  ∈ M3×3 (F ). 0

Show that Ak+2 = Ak + A2 − I for all positive integers k. Exercise 416 Let n be a positive integer and let F be a field. Let A, B ∈ Mn×n (F ) satisfy A + B = I. Show that AB = O if and only if A = A2 and B = B 2 . Exercise 417 Let n be a positive integer and let (K, •) be an associative unital algebra over a field F . Define a new operation on Mn×n (K), called the Schur product (sometimes also called the Hadamard product, especially in the context of statistics), by setting [vij ] [wij ] = [vij • wij ], for all 1 ≤ i, j ≤ n. Is (Mn×n (K), +, ) an F -algebra? Is it associative? Is it unital? When is it commutative? Exercise 418 Let n be a positive integer and for each A = [aij ] ∈ Mn×n (R), let µ(A) = max1≤i,j≤n |aij |. Show that µ(A2 ) ≤ nµ(A)2 for all A ∈ Mn×n (R).

158


Exercise  419 Let F be a field. Find a matrix A ∈ M3×3 (F ) satisfying 0 1 0 A2 =  0 0 0  or show that no such matrix exists. 0 0 0 ! 0 c AT = Exercise 420 Find a matrix A ∈ M2×2 (Q) satisfying A c 0 ! 2c 0 for all c ∈ Q. 0 − 2c Exercise 421 Let F be a field and let n be a positive integer. that H11 AH11 BH11 = H11 BH11 AH11 for all A, B ∈ Mn×n (F ).

Show

Exercise 422 Let F be a field and n be a positiveinteger. Show that let n n n n for all A, B ∈ i=1 j=1 Hij AHji B = B i=1 j=1 Hij AHji Mn×n (F ). Exercise 423 Is the set    1  1 1 0  0 0 0 , 0  0 0 0 0

1 0 0

  1 0 0 , 1 0 0

0 1 0

  0 0 0 , 1 0 0

0 1 0

 0  1   0

of matrices in M3×3 (Q) closed under taking products? Exercise 424 Find infinitely-many triples (A, B, C) of nonzero matrices in M3×3 (Q), the entries of which are nonnegative integers, satisfying the condition A3 + B 3 = C 3 . Exercise 425 Let F be a field. Find a matrix A ∈ M4×4 (F ) satisfying A4 = I = A3 . Exercise 426 Let n be a positive integer and let F = GF (p) for some prime integer p. Show that for any A ∈ Mn×n (F ) there exist positive integers k > h satisfying Ak = Ah . Would this also be true if we chose F = Q? Exercise 427 Let A = [aij ] ∈ M2×2 (C) be a matrix satisfying √ 1 [a11 + a22 ] = a11 a22 − a12 a21 . 2 Show that there exist four distinct matrices B ∈ M2×2 (C) satisfying B 2 = A. Exercise 428 Let c be a given complex number. Find the set of all matrices A ∈ M2×2 (C) satisfying (A − cI)2 = O.




3 − 4c Exercise 429 Show that  −1 + 2c −3 + 2c complex numbers c.

159

2 2 − 4c 2 − 4c 2c −1 + 2c  = I for all −3 + 2c −2 + 2c

Exercise 430 Show that there is no matrix A ∈ M2×2 (C) satisfying ! 0 1 2 A = . 0 0 Exercise 431 Let n be a positive integer and let F be a field. How many matrices A = [aij ] ∈ Mn×n (F ) having entries in {0, 1} satisfy the condition that each row and each column contain exactly one 1. Exercise 432 Show that for an integer n ≥ 4 and for a field F there exist matrices A and B in Mn×n (F ) satisfying A2 = B 2 = O but AB = BA = O. Exercise 433 Let F = GF (2) and let F be a field of characteristic other than 2. Define a function ϕ : M2×2 (F ) → M2×2 (F ) as follows: if A = [aij ] ∈ M2×2 (F ) then set ϕ(A) = [bij ], where

1 if aij = 0 . bij = 0 otherwise Is ϕ(A + A ) = ϕ(A) + ϕ(A ) for all A, A ∈ M2×2 (F )? Is ϕ(AA ) = ϕ(A)ϕ(A ) for all A, A ∈ M2×2 (F )? Exercise  1 0 A 1 1 0 0

434 Find   0 0 = 1

a matrix I = A ∈ M3×3 (Q) satisfying     1 0 0 1 0 0 1 1 1 0  A and A  0 1 0  =  0 0 0 1 0 1 1 0

0 1 1

 0 0  A. 1

Exercise 435 For each real number a, find a matrix B(a) ∈ M2×2 (R) ! ! cos(a) − sin(a) 1 0 satisfying = B(a) . sin(a) cos(a) sin(a) 1 ! 5 7 Exercise 436 Let A = ∈ M2×2 (R). What is A1024 ? −3 −4 Exercise 437 Find all pairs (a, b) of rational numbers such that the ! 2a −a matrix A = ∈ M2×2 (Q) satisfies A2 = A. 2b −b Exercise 438 Let F be a field and let n be a positive integer. Show that there do not exist nonsingular matrices P, Q ∈ Mn×n (F ) satisfying P AQ = AT for all A ∈ Mn×n (F ).

160


Exercise 439 Let F be a field and let A, B ∈ Mn×n (F ) be a commuting pair of matrices, where B is nonsingular. Is (A, B −1 ) necessarily a commuting pair?

Exercise 440 Let F be a field. Is S =

a b c d

! a+c=b+d

an F -subalgebra of M2×2 (F )? Exercise 441 Let F be a field. Given an element a of F, show that !2 a b = I in M2×2 (F ). there exist elements b, c, d ∈ F such that c d Exercise 442 Find all rational numbers a, b and d satisfying the !2 a b = I in M2×2 (Q). condition that 1 d Exercise 443 Let F be a field and let K be the subset of M3×3 (F ) consisting of O and of all of the upper-triangular matrices [aij ] satisfying 0 = a11 = a22 = a33 . Is K an F -subalgebra of M3×3 (F )? Is it a field? Exercise 444 Let F = GF (p), where p is a prime integer, and let K be the subset of M2×2 (F ) consisting of all matrices of the form ! a b , where a, b ∈ F. Show that K, together with the operations −b a of matrix addition and multiplication, is a field when p = 3 and is not a field when p = 5. What happens when p = 7? Exercise 445 Let n be a positive integer, let F be a field, and let O = A, B ∈ Mn×n (F ). Show that there exists a matrix C ∈ Mn×n (F ) satisfying ACB = O. Exercise 446 Find all matrices A,B ∈ M2×2 (R), the entries of which ! 1 1 are nonnegative integers, which satisfy AB = . 0 1 Exercise 447 Let V = M3×3 (Q). For each rational number t, let   0 1 3 αt : V → V be the linear transformation A → A  t 0 0  . Is 0 −1 4 the function t → αt a linear transformation from Q to End(V ), both considered as vector spaces over Q?


161

Exercise 448 Let n be a positive integer, let F be a field, and for some fixed c ∈ F , let A = [aij ] be the matrix in Mn×n (F ) defined by

c when i + j is even aij = . 0 otherwise Show that the subset {A, A2 , A3 } of Mn×n (F )  0  1 Exercise 449 Let F = GF (2) and let A =   0 0

is linearly dependent.  0 0 1 0 0 1   ∈ M4×4 (F ). 1 0 0  0 1 0

Let L = {O} ∪ {Ai | i ≥ 0} ⊆ M4×4 (F ). Show that L is closed under addition. Is L, under the usual definitions of addition and multiplication of matrices, a field? Exercise 450 ! Let K be the set of all matrices in M2×2 (Q) of the form a −3b . Show that K is a subalgebra of M2×2 (Q) which is in fact b a a field. Exercise 451 Find ! the set of all matrices A ∈ M2×2 (Q) which satisfy 1 1 2 . A +A= 1 1 ! 0 1 Exercise 452 Let A = ∈ M2×2 (Q) and let B and C be −1 0 matrices in M2×2 (Q) satisfying AB = BA and AC = CA. Show that BC = CB. Exercise 453 Find infinitely-many matrices A ∈ M3×3 (Q) satisfying     1 1 −1 2 1 0 2 0 1  =  0 1 − 32  . A 2 3 −1 3 0 0 0   1 −1 −1 1 −1  ∈ M3×3 (Q). Find functions Exercise 454 Let A =  −1 −1 −1 1 f and g from the set of all positive integers to Q satisfying the condition   f (n) g(n) g(n) that An =  g(n) f (n) g(n)  for all n ≥ 1. g(n) g(n) f (n) Exercise 455 Let F = GF (2). Do there exist matrices A = [aij ] and B = [bij ] in M2×2 (F ) satisfying a11 + a22 = 1, b11 + b22 = 0, and AB = I?

162


Exercise 456 Let F be a  1 M3×3 (F ) of the form  a 0

field and let G be the set of all matrices in  0 0 0 0  , where a, b ∈ F. Is G closed under 0 b

matrix multiplication? Does there exist a matrix J in G satisfying the condition that AJ = A for all A ∈ G? If such a matrix J exists, is it necessarily true that JA = A for all A ∈ G? Exercise 457 Let n be a positive integer and let F

be a field. Let ! I A and O I

A and B be matrices in Mn×n (F ) of the form ! I B respectively, where A and B are (not-necessarily square) O I matrices of the same size. Find necessary conditions for A and B to satisfy AB = BA. Exercise 458 Let F be a field and let A, B ∈ M2×2 (F ). Show that (AB − BA)2 is a diagonal matrix. Exercise 459 Let n be a positive integer and let F be a field. Let A ∈ Mn×n (F ) be a diagonal matrix having distinct entries on the diagonal. Let B ∈ Mn×n (F ) be a matrix satisfying AB = BA. Show that B is also a diagonal matrix. Exercise 460 Let n be a positive integer and let F be a field. For each integer −n < t < n, let Dt (F ) be the set of all matrices A = [aij ] ∈ Mn×n (F ) satisfying the condition that aij = 0 when j = i + t. Thus, for example, D0 (F ) is the set of all diagonal matrices in Mn×n (F ). If A ∈ Dt (F ) and B ∈ Ds (F ), does there necessarily exist an integer −n < u < t such that AB ∈ Du (F )? 

  1 2 3 1 Exercise 461 Let A =  −1 −2 −3  and B =  0 2 4 6 0

2 0 0

 3 0  0

be

matrices in M3×3 (R). Find infinitely-many lower-triangular matrices C satisfying A = CB. Exercise 462 Let n be a positive integer and let F be a field. Let A1 , . . . , An be upper-triangular matrices in Mn×n (F ) satisfying the condition that the (i, i)-entry in Ai is equal to 0 for 1 ≤ i ≤ n. Show that A1 · . . . · An = O.


163

Exercise 463 Let F be a field in which we have elements a = 0 and b. Show that there exists an upper-triangular matrix C ∈ M2×2 (F ) satisfying ! ! 0 a 0 b C= . Is C necessarily unique? 0 0 0 0 Exercise 464 Let F be a field. Find an element A of M2×2 (F ) AT A. satisfying AAT = Exercise 465 Let F be a field and let n > 1. If a matrix A ∈ Mn×n (F ) satisfies AAT = O, does it necessarily follow that AT A = O? Exercise 466 Let n be a positive integer, let F be a field, and let A ∈ Mn×n (F ) satisfy the condition A = AAT . Show that A2 = A. Exercise 467 Let n be a positive integer, let F be a field, and let A, B ∈ Mn×n (F ) be symmetric matrices. Is ABA necessarily symmetric? Exercise 468 Let n be a positive integer and let F be a field. If A ∈ Mn×n (F ) is symmetric, is Ah symmetric for all h > 1?

! ! !1 −2 1 3 −1 1 Exercise 469 Show that , , forms −2 1 3 6 1 −3 a basis for the subspace of M2×2 (Q) consisting of all symmetric matrices. T Exercise ! 470 Does there exist a matrix A ∈ M2×2 (R) satisfying AA = 1 9 ? 9 1

Exercise 471 Given real numbers a, b, and c,   0 0 0 −1 a b c 1  0  1 0 0 0 0 −1 a  such that   0 −1 a b  0 d 0 0 −1 a b c 0 0 1 0

find all real numbers d    is symmetric. 

Exercise 472 Find a matrix B ∈ M2×2 (Q) such that the Nievergelt’s matrix equals B T B.  −1 1 2 −3 2  in M3×3 (R). Exercise 473 Calculate  0 1 0 0 1  −1 a 1 1 Exercise 474 Let a ∈ R{1, −2}. Calculate  1 a 1  ∈ M3×3 (R). 1 1 a   −3 4 0 5 −2  ∈ Exercise 475 Does there exist an a such that  8 a −7 6 M3×3 (R) is singular?

164


Exercise 476 Let n be a positive integer. Each complex number c defines a matrix A(c) = [aij ] ∈ Mn×n (C) given by aij = c(i−1)(j−1) for all 1 ≤ i, j ≤ n. If w = e2πi/n ∈ C, show that A(w) is nonsingular and satisfies A(w)−1 = n1 A(w−1 ). Exercise 477 Let n be a positive integer and let F be a field. Given a matrix B ∈ Mn×n (F ), do there exist vectors u, v ∈ F n such that the ! B −Bv is nonsingular? matrix −uT B uT Bv   1 − a2 1 − a 0 0 1 − a2 1 − a  ∈ M3×3 (C) nonExercise 478 Is the matrix  1−a 0 1 − a2 √ 1 1 singular, where a = − 2 + 2 −3 ∈ C. Exercise 479 Let n be a positive integer and let F be a field. If A ∈ Mn×n (F ) nonsingular, is the same necessarily true for A + AT ? Exercise 480 Let n be a positive integer and letF be a field. Let n A = [aij ] ∈ Mn×n (F ) satisfy the condition that i=1 aij = 1 for all 1 ≤ j ≤ n. Show that the matrix I − A is singular. Exercise 481 Let n be a positive integer and let F be a field. If A ∈ Mn×n (F ) is a Markov matrix, is A−1 necessarily a Markov matrix? Exercise 482 Let n be a positive integer and let F be a field. For A ∈ Mn×n (F ), show that A2 is nonsingular if and only if A3 is nonsingular. Exercise 483 Let F = GF (p), where p is a prime integer, and let n be a positive integer. What is the probability that a matrix in Mn×n (F ), chosen at random, is nonsingular? ! 0 −1 Exercise 484 Let P = ∈ M2×2 (R) and let A and Q be 1 −1 nonsingular matrices in M2×2 (R). Set B = AQ−1 P Q. Show that B is nonsingular and A−1 + B −1 = (A + B)−1 . Exercise 485 Show that there are infinitely-many matrices A ∈ M2×2 (Q) satisfying A = A−1 . Exercise 486 Let F = GF (2). Is the sum of all nonsingular matrices in M2×2 (F ) nonsingular? Exercise 487 Let F be a field and let U be the set of all nonsingular matrices in M2×2 (F ). Is the function θ : U → U defined by θ : A → A2 a permutation of U ?


165

Exercise 488 Let n be a positive integer, let F be a field, and let A ∈ ! A11 A12 , M2n×2n (F ) be a matrix which can be written in the form A21 A22 where each Aij ∈ Mn×n (F ) is nonsingular. Is A necessarily nonsingular? Exercise 489 Let n be a positive integer and let F be a field. Do there ! A2 AB ∈ exist matrices A, B ∈ Mn×n (F ) such that the matrix BA B 2 M2n×2n (F ) is nonsingular? Exercise 490 Let n be a positive integer and let F A, B ∈ Mn×n (F ) with A nonsingular, show that

be a field. For

(A + B)A−1 (A − B) = (A − B)A−1 (A + B). Exercise 491 Let n and p be positive integers and let F be a field. Let A ∈ Mn×n (F ) and let B, C ∈ Mn×p (F ) be matrices satisfying the condition that A and (I + C T A−1 B) are nonsingular. Show that A + BC T is nonsingular, and that −1 A + BC T = A−1 − A−1 B(I + C T A−1 B)−1 C T A−1 . Exercise 492 Let n be a positive integer and let F be a field. If   0  ..   .  = v ∈ F n , show that there exists a nonsingular matrix in Mn×n (F ) 0 the last row of which is v. Exercise 493 Let F be a field. Show that every nonsingular matrix in ! 0 1 , M2×2 (F ) can be written as a product of matrices of the form 1 0 ! ! 1 1 a 0 , or for a ∈ F. 0 1 0 1   1 0 t Exercise 494 For each real number t, let A(t) =  −t 1 − 12 t2  ∈ 0 0 1 M3×3 (R). Show that each such matrix is nonsingular and that the set of all such matrices is closed under taking products. Exercise 495 Let n be a positive integer and let F be a field. Let A ∈ Mn×n (F ) be a matrix for which there exists a positive integer k satisfying Ak = O. Show that the matrix I − A is nonsingular and find (I − A)−1 .

166


Exercise 496 Let n be a positive integer and let F be a field. Let A ∈ Mn×n (F ) be a matrix for which there exists a matrix B ∈ Mn×n (F ) satisfying I + A + AB = O. Show that A is nonsingular. Exercise 497 Let n be a positive integer and let F be a field. Let A, B ∈ Mn×n (F ) satisfy the condition that A and A+B are nonsingular. Show that I + A−1 B is nonsingular and that (I + A−1 B)−1 = (A + B)−1 A. Exercise 498 Find matrices A and B in M2×2 (R) satisfying A2 = B 2 = O and that A + iB is a nonsingular matrix in M2×2 (C).   1 0 b Exercise 499 Let F be a field and let A =  0 1 0  ∈ M3×3 (F ), a 0 1 where ab = 1. Show that A is nonsingular and calculate A−1 . Exercise 500  c 1 0 0  0 c 1 0   0 0 c 1 0 0 0 c A−1 .

Let c = 0 be an element of a field F    ∈ M4×4 (F ). 

Show that

A

and let A =

is nonsingular and find

Exercise 501 Let n > 1 and let B ∈ Mn×n (Q) be the matrix all of the entries of which are equal to 1. Show that there exists a matrix A ∈ Mn×n (Q) satisfying the condition that A + cB is nonsingular for all rational numbers c. Exercise 502 Let n > 1 and let B ∈ Mn×n (Q) be the matrix all of the entries of which are equal to 1. Find a rational number t such that (I − B)−1 = I − tB. Exercise 503 Let n be a positive integer and let A = [aij ] ∈ Mn×n (R) be the matrix defined by aij = min{i, j} for all 1 ≤ i, j ≤ n. Show that A is nonsingular. Exercise 504 Let A = [aij ] ∈ M4×4 (R) be the matrix defined by

2 if i = j − 1 . aij = 1 otherwise Show that A is nonsingular and calculate A−1 . Exercise 505 For each real number a, let G(a) =

cos(a) sin(a) − sin(a) cos(a)

! ∈

M2×2 (R). Given real numbers a, b, and c, show that G(a, b, c) = ! G(a) G(b) ∈ M4×4 (R) is nonsingular, and find G(a, b, c)−1 . O G(c)


167

Exercise 506 Find a singular matrix in M3×3 (Q) the entries of which (in some order) are the integers 1, 2, . . . , 9. Exercise 507 Let n be a positive integer and let F be a field. Given elements b, c ∈ F, let A = [aij ] ∈ Mn×n (F ) be the matrix defined by

b if i = j . aij = c otherwise Find necessary and sufficient conditions for A to be nonsingular. ! 0 1 Exercise 508 Let F be a field and let D = ∈ M2×2 (F ). −1 0 Let A ∈ M2×2 (F ) satisfy the condition that AT DA = D. Show that A is nonsingular. Exercise 509 Let n be a positive integer and let F be a field. Is the set of all singular matrices in Mn×n (F ) closed under taking products? Exercise 510 Let n be a positive integer, let F be a field, and let A, B ∈ Mn×n (F ). Show that A and B are both nonsingular if and only ! A O if the matrix ∈ M(2n)×(2n) (F ) is nonsingular. O B   1 1 1 Exercise 511 Let A =  1 1 1  ∈ M3×3 (Q). Find a rational num1 1 1 ber c satisfying (I − A)−1 = I − cA. Exercise 512 Write the matrix

1 −2 2 2

! ∈ M2×2 (R) as a product of

elementary matrices. Exercise 513 Find the change of basis matrix from the canonical basis B       1 1   1 of R3 to the basis D =  1  ,  1  ,  0  and the change of   1 0 0 basis matrix from D to B.

! a a Exercise 514 Let G = 0 = a ∈ R . Show that there a a exists a matrix E ∈ G satisfying the condition that EA = A = AE for all A ∈ G. For each A ∈ G, show that there exists a matrix A‡ ∈ G satisfying AA‡ = E = A‡ A. Exercise 515 Let F be a field. Given matrices A, B ∈ M2×2 (F ), find the set of all matrices C ∈ M2×2 (F ) satisfying (AB − BA)C = C(AB − BA).

168


Exercise 516 Let F be a field and let G be the set of all automorphisms of F 2 which are represented with respect to the canonical basis by a matrix ! a b . Is G a group of automorphisms of F 2 ? of the form 0 a−1 Exercise 517 Let G be the set of all automorphisms of Q2 which are represented with respect to the canonical basis by a matrix of the form ! a b , where a, d > 0. Is G a group of automorphisms of Q2 ? 0 d Exercise 518 Let W1 ⊆ W2 ⊆ . . . ⊆ Wn be a fixed sequence of subspaces of a vector space V finitely generated over a field F, If α ∈ Aut(V ), we say that given sequence is an α-fan if and only if each of the Wi is invariant under α. Show that G = {α ∈ Aut(V ) | the given sequence is an α-fan} is a group of automorphisms of V. Exercise 519 For any real number t and any positive integer n, we can define the matrix P (n, t) ∈ Mn×n (R) to equal the identity matrix I in the case t = 0 and otherwise to equal the matrix [pij ] defined by

pij =

i−10 i−j j−1 t

if i < j . otherwise

Show that P (n, s)P (n, t) = P (n, s + t) for all s, t ∈ R. show that each matrix P (n, t) is nonsingular.

In particular,

Exercise 520 Let F be a field and let X be an indeterminate over F . Find matrices P and Q in M2×2 (F [X]) such that the matrix ! 1 + X2 X P Q is a diagonal matrix. X 1+X Exercise 521 Let n be a positive integer and let α : Mn (C) → M2n (R) be the function defined by   a b c d !  −b −a −d c  a + bi c + di . α: →   e e + f i g + hi f g h  −f e −h g Show that α is a linear transformation of vector spaces over R. Is it a homomorphism of unital R-algebras?

10 Systems of linear equations

The classical problem of linear algebra is to find all solutions (if any exist) to a system of linear equations in n unknowns of the form a11 X1 + . . . + a1n Xn a21 X1 + . . . + a2n Xn ... ak1 X1 + . . . + akn Xn

= b1 = b2 = bk

where the aij and the bi are scalars belonging to some field F and the Xj are variables which take values in F. Example: Let a < b be real numbers and let V = C(a, b). If W is a subspace of V of dimension n then the interpolation problem of V is the following: given a function f ∈ V and given real numbers a ≤ t1 < . . . < tn ≤ b, find a function g ∈ W satisfying f (tj ) = g(tj ) . . , gn } of W then we want for 1 ≤ j ≤ n. If we are given a basis {g1 , . n to find real numbers c1 , . . . , cn satisfying i=1 ci gi (tj ) = f (tj ) for all 1 ≤ j ≤ n. In other words, we want to solve a system of linear equations of the above form, where k = n, aij = gj (ti ) and bi = f (ti ) for all 1 ≤ i, j ≤ n. Example: In Proposition 4.2 we noted that if F is a field and if f (X) and g(X) = 0 are elements of F [X], then there exist unique polynomials u(X) and v(X) in F [X] satisfying f (X) = g(X)u(X) + v(X) and 169

170

10. Systems of linear equations

k n deg(v) < deg(g). If we set g(X) = i=0 ai X i and f (x) = i=1 bi X i , n−k then the coefficients of u(X) = i=0 ci X i are found by solving the system of linear equations ak Y0 + ak−1 Y1 + . . . + a0 Yk ak Y1 + ak−1 Y2 + . . . + a0 Yk+1 ... ak Yn−k−1 + ak−1 Yn−k ak Yn−k

= bk = bk−1 = bn−1 = bn

by any of the methods we will discuss. Example: Sometimes we can transform systems of nonlinear equations into systems of linear equations. For example, suppose that we want to find positive real numbers r1 , r2 , and r3 satisfying the following nonlinear system of equations: r1 r2 r3 r13 r22 r32 r3 /r1 r2

= =

1 27.

=

81

Since each of the integers on the right is a power of 3, we can take the logarithm to the base 3 of both sides of each equation. Setting Xi = log3 (ri ) for 1 ≤ i ≤ 3, the system now becomes linear X 1 + X2 + X3 3X1 + 2X2 + 2X3 −X1 − X2 + X3

= =

0 3

=

4

and this has a unique solution (which we can find by methods to be discussed in this chapter) X1 = 3, X2 = −5, and X3 = 2, showing that the original system has a solution r1 = 27, r2 = 1/243, and r3 = 9. A system of linear equations of the above form is homogeneous if and only if bi = 0 for all 1 ≤ i ≤ k; otherwise it is nonhomogeneous. At this stage, we do not yet know answers to the following questions: (1) Does a given system of linear equations have a solution? (2) If it has a solution, is that solution unique? (3) If the solution is not unique, can we characterize the set of all solutions? (4) If there are solutions, how do we compute them efficiently? In order to answer these questions, we have to move to the language of matrices. The use of matrices for this purpose was developed in Europe in the 19th century by Cayley, Sylvester, and Laguerre. However, the real pioneers were the Chinese and Japanese mathematicians. During the time


171

of the Han dynasty in China, around 2000 years ago, the classical book Nine Chapters on the Mathematical Art (Jiuzhang Suanshu, ) presented a method for solving systems of linear equations using matrices. This was later expanded by the Japanese mathematician Seki1 . How is this done? Let us write the above system in the form 

a11  ..  . ak1

... ...

   a1n X1 ..   ..  =  .  .   Xn akn

 b1 ..  . .  bk

The matrix A = [aij ] ∈ Mk×n (F ) is the coefficient matrix of the   b1 ( )   A w ∈ system. If we set w =  ...  ∈ F k , then the matrix bk Mk×(n+1) (F ) is called the extended coefficient matrix of the system.   d1   The set of all vectors v =  ...  ∈ F n satisfying Av = w is the dn solution set of the system. This is clearly equal to α−1 (w), where α : F n → F k is the linear transformation satisfying ΦBD (α) = A, where B and D are the canonical bases of F n and F k respectively. In particular, if the system is homogeneous then its solution set is just the kernel of α, and is called the solution space of the system. We note the following simple but important point: if F is a subfield of a field K and if k and n are positive integers, then any matrix A in Mk×n (F ) also belongs to Mk×n (K) and any vector v ∈ F n also belongs to K n . Therefore, if w ∈ F k , any element of the solution set of Av = w, considered as a system of linear equations over F, remains a solution when we consider this as a system of linear equations over K.

1

Edmond Laguerre, a 19th centry French mathematician, wrote an important book on systems of linear equations in 1867. Takakazu Seki Kowa was a 17th century Japanese mathematician, the son of a samurai warrior family, who developed matrix-based methods based on old Chinese texts.

172


(10.1) Proposition: The solution set of a homogeneous system of linear equations in n unknowns is a subspace of F n .

Proof: This is a direct consequence of Proposition 6.4.

For nonhomogeneous systems, the situation is a bit more complicated. (10.2) Proposition: Let AX = w be a nonhomogeneous system of linear equations in n unknowns over a field F and let v0 ∈ F n be a solution to this systems. Then the solution set of the system is the set of all vectors in F n of the form v0 + v, where v is a   0   solution to the homogeneous system AX =  ...  . 0 Proof: This is an immediate consequence of Proposition 6.6.

We should emphasize that the solution set of a nonhomogeneous system of linear equations is not a subspace of F n but rather an affine subset of that space. Example: If we identify R2 with the Euclidean plane by associating ! a each vector with the point with coordinates (a, b), then we see its b subspaces of of dimension 1 are precisely the straight lines going through the origin. The solutions of linear equations of the form a1 X1 + a2 X2 = b, where b = 0, and at least one of the ai is also nonzero, are the straight lines in the plane which do not go through the origin. We are still left with the question of how to actually find a solution to a system of linear equations. Here we can distinguish between two approaches: (1) Direct methods. These methods involve the manipulation of the matrix A, either replacing it with another matrix which is easier to work with or factoring it into a product of matrices which are easier to work with, and thus reducing the difficulty of the problem. (2) Iterative methods. These methods involve selecting a likely solution for the system and then repeatedly modifying it to obtain a sequence of vectors which (hopefully) will converge to an actual solution to the system. Such methods work, of course, only if our vector space is one in which the notion of convergence is meaningfully defined. As we shall see, this is possible when the field of scalars equals R or C.


173

We begin by looking at direct methods. Let P be a nonsingular matrix in Mk×k (F ). A vector v ∈ F n is a solution to the system AX = w over F if and only if it is a solution to the system (P A)X = P w. In particular, this is true for elementary matrices. Thus, given a system of linear equations, we can change the order of the equations, multiply one of the equations by a nonzero scalar, or add a scalar multiple of one equation to another, without changing the solution set of the system, so long as we do the same thing on both sides of the equal sign. In order (to do this) efficiently, it is best to work with the extended coefficient matrix A w and perform elementary operations on it to reduce it to a convenient form. Which form should we choose? Let F be a field, let k and n be positive integers, and let B = [bij ] ∈ Mk×n (F ). The matrix B is in row echelon form if and only if the following conditions are satisfied: (1) If 1 < s ≤ k then bs,j = 0 for all 1 ≤ j < s; (2) If 1 ≤ s ≤ k and 1 ≤ t ≤ n satisfy the condition that bsj = 0 for all 1 ≤ j < t, then bij = 0 for all s < i ≤ k and all 1 ≤ j ≤ t. 

1  0 Example: The matrices   0 0

6 9 0 0

7 2 0 0

7 1 2 0 

1  0 are in row echelon form. The matrix   0 0 echelon form.

  1 8  0 1   and   0 2  1 0 5 0 0 0

2 1 1 0

9 5 0 0

0 0 0 0 

0 0 0 0

0 2 0 0

 0 6   0  0

0 4   is not in row 1  7

Example: If n is a positive integer and if B ∈ Mn×n (F ) is in row ech  1 0 2 7  0 0 3 8   elon form, then B is surely upper triangular. However,   0 0 9 0  0 0 0 5 is an upper-triangular matrix which is not in row echelon form. We claim that for any matrix A = [aij ] ∈ Mk×n (F ) is row equivalent to a matrix in row echelon form. By Proposition 9.4, this is equivalent to saying that A can be transformed into a matrix in row echelon form by a series of elementary operations, as follows: (1) Find the leftmost column of A which has a nonzero entry and interchange rows if necessary, so that this entry is in the first row. Thus we now have a matrix A in which a1h = 0 and aij = 0 for all 1 ≤ i ≤ k and all 1 ≤ j < h.

174


(2) For each 1 < i ≤ k, if aih = 0 then we multiply the first row by −aij a−1 1h and add it to the ith row, which creates a new row in which the (i, h)-entry is equal to 0. Thus, we now have a matrix in which aih = 0 for all 1 < i ≤ k. (3) Now consider the submatrix of A from which we deleted the first row and the first h columns, and repeat the above procedure.



1 Example: Let us begin with the matrix A =  2 1

 2 3 1 1 4 2  ∈ −1 1 1

M3×4 (R). We already have a11 = 0. Multiplying the first row by −2   1 2 3 1 and adding it to the second row, we obtain  0 −3 −2 0  and 1 −1 1 1 then multiplying the first row by −1 and adding it to the third row,   1 2 3 1 we obtain  0 −3 −2 0  . We also already have a22 = 0. Multi0 −3 −2 0 plying the second row by −1 and adding it to the third row, we obtain   1 2 3 1  0 −3 −2 0  , and this is in row echelon form. 0 0 0 0

If A = [aij ] ∈ Mk×n (F ) is a matrix in row echelon form, and if the hth row of A contains nonzero entries, then the leftmost nonzero entry of the row is the leading entry. The matrix A is in reduced row echelon form if it is in row echelon form and, in addition, satisfies the following additional conditions: (1) The leading entry in each nonzero row is equal to 1; (2) If ahj is a leading entry, then aij = 0 for all i = h. Any matrix in row echelon is row-equivalent to one in reduced row echelon form; that is to say, such a matrix can be converted to one in reduced row echelon form by performing additional elementary operations: first we multiply each nonzero row by the multiplicative inverse of its leading entry, to obtain a matrix in which the leading entry of each nonzero row equals 1. Then, if ahj is a leading entry and if i < h, we multiply the hth row by −aij and add it to the ith row, which will give us a matrix with the (i, j)-entry equal to 0. The reduced row echelon form of any given matrix is clearly unique.




1 Example: Let us go back and look at the matrix  0 0

2 −3 0

175

 3 1 −2 0  0 0

in row echelon form. The leading entry of the first row  to  is already equal 1 2 3 1 1. Multiplying the second row by − 13 to obtain,  0 1 23 0  , a 0 0 0 0 matrix in which the leading entry of the second row is equal to 1 as well. Now multiply the second row by −2 and add it to the first row, to obtain   1 0 83 1  0 1 2 0  , which is in reduced row echelon form. 3 0 0 0 0 Now let us return to the system of linear equations AX = w in n unknowns and consider methods of solution. The most well-known is Gaussian elimination or the Gauss-Jordan method.2 In this method, we elementary operations on the extended coefficient matrix ( first perform ) A w to bring it to reduced row echelon form. Having done this, we now have a new system of linear equations A X = w , the solution set of which is the same as that of the original system. Let t be the greatest integer i such that the ith row has nonzero entries. There are several possibilities: (1) bt = 0 but atj = 0 for all 1 ≤ j ≤ n. Then the system has no solutions and we are done. (2) There is precisely one index j such that atj = 0. Then this must in fact be the leading entry of the tth row and so atj = 1. This means that in any element of the solution set of the system we must have the jth entry equal to bj . We can therefore substitute bj for Xj in each of the other equations, and reduce the system to one of equations of n − 1 unknowns. (3) There are several indices j such that atj = 0, say those in columns h1 < h2 < · · · < hm . Then ath1 is the leading entry of the tth

2

Carl Friedrich Gauss, who lived in Germany at the beginning of the 19th century, is considered to be the leading mathematician of all times, as well as a physicist and astronomer of the first rank. He developed this method in connection with his work in astronomy in 1809. Gaussian elimination first appeared in print in a handbook by German geodicist Wilhelm Jordan, who applied the method to problems in surveying.

176


row and so equals 1. Moreover, for any values z1 , . . . , zm we substitute , we will get a solution to the system with these values for Xh2 , . . . , Xh m m and with bt − s=2 zs substituted for Xh1 . Thus we can consider the zi as parameters of a general solution and again reduce the system to one in a smaller number of unknowns. (4) Having reduced the system, we now recursively apply the previous steps until the system is solved. Strassen’s insight that Gaussian elimination may not be the optimal method of solving systems of linear equations, as had been previously thought, led to the development of his method of matrix multiplication. Example: Let us consider the system of linear equations 3X1 + 2X2 + X3 −2X1 + X2 − X3 2X1 − X2 + 2X3

=

0

= =

2 −1

over the field R. The extended coefficient matrix of this system is   3 2 1 0  −2 1 −1 2  2 −1 2 −1   1 0 1 23 3 and this is row equivalent to the matrix  0 7 −1 6  in row echelon 0 0 1 1   1 0 0 −1 1  in form, which is in turn row equivalent to the matrix  0 1 0 0 0 1 1 reduced row echelon form. Thus we see that the solution set of the system    −1   1  . is   1 Example: Let us consider the system of linear equations X1 + X2 X1 − X 2 −X1 + 2X2

=

1

= =

3 −2

over the field R. The extended coefficient matrix of this system equals     1 1 1 1 1 1  1 −1 3  , and this is row equivalent to the matrix  0 −2 2  −1 2 −2 0 0 2




1 in row echelon form, which is row equivalent to the matrix  0 0

177

0 1 0

 0 0  1

in reduced row echelon form. Therefore this system has no solutions at all. Example: Let us consider the system of linear equations X1 + 2X2 + X3 2X1 + 4X2 + 3X3 3X1 + 6X2 + 4X3

=

−1

= =

3 2

over the field R. The extended  1  2 3

coefficient matrix of this system is  2 1 −1 4 3 3  6 4 2   1 2 1 −1 5  in row echelon and this is row equivalent to the matrix  0 0 1 0 0 0 0   1 2 0 −6 5  in form, which is in turn row equivalent to the matrix  0 0 1 0 0 0 0 reduced row echelon form. From the second row we see that we must have X3 = 5. From the first row we have X1 + 2X2 = −6 and so, for each value X2 = z, we have a solution with X1 = −6 − 2z. Therefore the     −6 − 2z    z∈R . z solution set to our system is   5 We note that if A ∈ Mk×n (F ) then the number of arithmetic operations needed so solve a system of linear equations of the form AX = w using Gaussian elimination, is no more than 16 k(k ( ) −1)(3n−k −2) if k < n 1 and no more than 6 n 3kn + 3(k − n) − n2 − 2 otherwise3 . Of course, if

3

The first computer program to solve a system of linear equations by Gaussian elimination was written by Lady Augusta Ada Lovelace, a student of

178


the matrix A is of a special form, this procedure can be much faster. For example, if A ∈ Mn×n (F ) is a tridiagonal matrix, then a system of equations of the form AX = w can be solved using 3n additions/subtractions and 5n multiplications. Gaussian elimination can also be used to check if a set of vectors in F k is linearly independent. Let {v1 , . . . , vn } be a set of vectors in F k , where   a1j   vj =  ...  for all j. We want to know if there exist scalars b1 , . . . , bn akj



 0 n  ..  in F, not all equal to 0, satisfying j=1 bj vj =  .  . In other 0 words, we want to know if the homogeneous systems of linear equations   0   AX =  ...  has a nonzero solution, where A = [aij ] ∈ Mk×n (F ). 0       1 3 −1       −3   1  −1        Example: Let us check if the subset  3  ,  6  ,  0       4 4 4 of Q4 is linearly dependent, and to do so we need to consider the matrix   1 3 −1 0  −1 −3 1 0  . A=  3 6 0 0  4 4 4 0   1 0 2 0  0 1 −1 0   in reduced This matrix is row equivalent to the matrix   0 0 0 0  0 0 0 0 row echelon form. Therefore the set of solutions to the homogeneous system      0  −2z     z  z∈Q AX =  ...  is so that if we pick one such   z 0 De Morgan and daughter of the poet Lord Byron, who developed software for Charles Babbage’s (never completed) mechanical computer in the 19th century. Her program was capable of solving systems of 10 linear equations in 10 unknowns.


179



 −2 nonzero element, say  1  , we see that 1 

      1 3 −1 0  −1   −3   1   0       (−2)   3 + 6 + 0 = 0 4 4 4 0

  , 

showing that the set is indeed linearly dependent.

If A ∈ Mk×n (F ) is a nonsingular matrix which can be written in the form LU, where L is lower triangular and U is upper triangular, then a system of linear equations of the form U X = w is easy to solve using Gaussian elimination, since U is already in row-echelon form. Moreover, since U must also be nonsingular, this system has a unique solution y = U −1 w. Then the system AX = w has a unique solution, which is also the solution to the system LX = y and that system too is easy to solve. We therefore see the importance of the LU -decomposition of matrices, assuming that one exists.

Given a matrix A ∈ Mk×n (F ), we define the column space of A to be the subspace of F k generated by the set of all columns of A. The dimension of the column space of A is called the rank of A. Moreover, there exists a linear transformation α : F n → F k satisfying the condition that ΦBD (α) = A, where B and D be the canonical bases of F n and F k respectively, and it is clear that the column space of A is just im(α). Similarly, we define the row space of A to be the subspace of M1×n (F ) generated by the rows of A. We will show that the dimension of this space is also equal to the rank of A.

(10.3) Proposition: Let F be a field, let k and n be positive   b1   integers, and let A ∈ Mk×n (F ) and let w =  ...  ∈ F k . Then bk the system of linear equations AX = w has a solution if and only if w belongs to the column space of A.

180




 d1   Proof: If v =  ...  is a solution of the system AX = w then dn  n

 a1j     .. w= dj  ...  = n . j=1 akj j=1 akj dj j=1

a1j dj

and so w is a linear combination we assume that there exist scalars    a1j d1 n  ..   .. j=1 dj  .  , then v =  . akj





n

of the columns of A. Conversely, if d1 , . . . , dn in F such that w =    is a solution of the given system.

dn

In particular, we get the following consequence of this result.

(10.4) Proposition: Let F be a field, let k and  b1  .. integers, and let A ∈ Mk×n (F ) and let w =  .

n be positive    ∈ F k . Then

bk the system of linear equations AX = w has a solution if and only if the rank of the coefficient matrix A is equal to the rank of the extended coefficient matrix.

Now let us return to the problem of identifying the solution sets of homogeneous systems of linear equations.

(10.5) Proposition: Let F be a field, let k and n be positive integers, and let A ∈ Mk×n (F ) be a matrix the columns of which are vectors y1 , . . . yn in F k . Assume these columns are arranged such that {y1 , . . . , yr } is a basis for the column space of A, for some r ≤ n. Moreover, for all r < h ≤ n, let us select scalars bh1 , . . . , bhn such that: (1) yh = bh1 y1 + . . . + bhr yr ; (2) bhh = −1; (3) bhj = 0 otherwise.


181



 bh1   For each r < h ≤ n, let vh =  ...  ∈ F n . Then {vr+1 , . . . , vn } bhn is a basis for the solution space of the homogeneous system of   0  ..  linear equations AX =  .  . 0 (Comment before the proof: Since {y1 , . . . , yn } is a set of generators for the column space of A, it contains a subset that is a basis. The assumption that this subset is {y1 , . . . , yr } is for notational convenience only.) Proof:

If r     equations is   

= n then the solution space of the system of linear  0   ..  and so the result is immediate. Hence let us  .   0   0 r  ..  bhj yj − yh =  .  assume that r < n. If r < h ≤ n, then Avh = j=1





0

0  ..  and so each vh belongs to the solution space of AX =  .  . Moreover, 0   0 n   cj vj =  ...  the set {vr+1 , . . . vn } is linearly independent, since if j=r+1

0

then for each r < h ≤ n we note that the hth entry on the left-hand side is −ch whereas the corresponding entry on the right-hand side is 0, proving that ch = 0 for all r < h ≤ n. We are therefore left to show that {vr+1 , . . . vn } is a generating set for the solution space of the given homogeneous system. And, indeed, let   d1 n   d h vh = w =  ...  be a vector in this solution space. Then w + 

d  n

h=r+1

e1  ..   .  , where er+1 = . . . = en = 0. Therefore, this vector belongs to en

182




 0   solution space of the system, and so eh yh =  ...  . However, since the h=q 0 r

set {y1 , . . . , yr } is linearly independent, this implies that e1 = . . . = er = 0 n as well. Therefore w = − dh vh , showing that {vr+1 , . . . vn } is a h=r+1

generating set for the solution space, as required.

As an immediate consequence of Proposition 10.5, we obtain the following result. (10.6) Proposition: Let F be a field, let k and n be positive integers, and let A ∈ Mk×n (F ). Then the dimension of the solution space of the homogeneous system of linear equations   0  ..  AX =  .  is n − r, where r is the rank of the coefficient 0 matrix A.

We are now ready to prove the characterization of rank which we mentioned before. (10.7) Proposition: Let F be a field, let k and n be positive integers, and let A ∈ Mk×n (F ). Then the rank of A equals the dimension of the row space of A. Proof: Let v1 , . . . vk be the rows of A, which generate a subspace of M1×n (F ). We can reorder these rows in such a way that {v1 , . . . vt } is a basis for the row space, for some 1 ≤ t ≤ k. This, as we know, does not change the solution space of the homogeneous system of linear   0   equations AX =  ...  and hence does not change the rank rA of A. 0 Let B ∈ Mt×n (F ) be the matrix obtained from A be deleting rows t + 1, . . . , k. The columns of B belong to F t and so the rank rB of B satisfies rB ≤ t, which implies that n − t ≤ n − rB . But we have already   0  ..  seen that the homogeneous systems of linear equations AX =  .  and 0


183



 0   BX =  ...  have the same solution space and so, by Proposition 10.6, 0 n − t ≤ n − rA . From this we conclude that rA ≤ t. We have thus shown that the rank of any matrix is less than or equal to the dimension of its row space. In particular, this is also true for AT . But the rank of AT is t, while the dimension of its row space is rA , and so we have t ≤ rA as well, proving equality.

Example: Let us find a basis for the solution space of the system of lin  ! X1 !  1 2 −3 1   X2  = 0 ear equations over R. We know that 1 1 1 1  X3  0 X4 ! 1 0 5 1 the coefficient matrix is row-equivalent to the matrix 0 1 −4 0 in reduced row echelon form, and this matrix has rank 2. Therefore the solution space of the system has dimension 4 − 2 = 2. Indeed, it is easy     −5 −1       0  4      to check that  1  ,  0  is a basis for this solution space.      0 1

Gaussian elimination requires an order of magnitude of n3 arithmetic operations to solve a system of n linear equations in n unknowns. This computational overhead is quite significant if n is large (say, over 10, 000), even with the use of supercomputers. As a result, there is considerable continuing research into finding faster methods of computation, especially in those cases in which we have additional information on the structure of the matrix of coefficients, originating in knowledge of the particular problem from which the system arose. Often this structural information is immediately noticeable, but sometimes it appears only after a sophisticated consideration of the problem.

Example: It is often possible to show that the matrix we are interested in, while not itself having a special structure, is equal to the product of two matrices having a special structure, a situation which arises in many mathematical models. Let us consider one such case. An n × n symmetric Toeplitz matrix is a matrix B = [bij ] ∈ Mn×n (R) satisfying the condition that there exist real numbers c0 , . . . , cn−1 such that bij = ch

184




1  2 whenever |i − j| = h. Thus, for example, the matrix   0 7

2 1 2 0

0 2 1 2

 7 0   2  1

is a symmetric Toeplitz matrix. Clearly the set of all symmetric Toeplitz matrices is a subspace of Mn×n (R). However, it is not a subalgebra, since the product of two such matrices need not be a symmetric Toeplitz matrix. They are also convenient to store in a computer, since we need keep in memory ony the n scalars c0 , . . . , cn−1 . Many mathematical models in economics are built around solving systems of linear equations of the form AX = w, where A is a product of two symmetric Toeplitz matrices.4 The proper use of mathematical techniques, and especially computational techniques, also depends very much on a deep understanding of the particular problem one is dealing with. Also, it is crucial to emphasize once again that any method we use to solve a system of linear equations on a computer will induce errors as a result of roundoff and truncation in our computations. With some methods – such as Gaussian elimination – these errors tend to accumulate, whereas with others they often cancel each other out, within certain limits. It is therefore necessary, especially when we are dealing with large matrices, to have on hand several methods of handling such systems of equations and to be able to keep track of the way in which errors can propagate in each of the different methods at one’s disposal.5

4 Otto Toeplitz was a 20th-century German mathematician who studied endomorphisms of infinite-dimensional vector spaces.

5 The problem of the numerical stability of computed solutions of systems of linear equations was the subject of considerable research in the early days of computers. Among the outstanding contributors were the Russian husbandand-wife team of Dimitri Konstantinovich Faddeev and Vera Nikolaevna Faddeeva.


185

We now turn to iterative methods of solution of systems of linear equations. For simplicity, we will assume that our field of scalars is always R. The basic idea is, as we have already noted, to guess a possible solution and then use this initial guess to compute a sequence of further approximations to the solution which, hopefully, will converge (in some topology) with relative rapidity. Usually, the initial guess is based on knowledge of the real-life problem which gave rise to the system of equations, something that can often be done with good accuracy. In very large and computationally-difficult situations (for example, weather prediction, chip design, large-scale economic models, computational acoustics, or the modeling the chemistry of polymer chains) one can even use Monte Carlo methods, based on statistical sampling and estimation techniques, to come up with an initial guess or even an approximate solution. To illustrate this approach, let us consider the problem of solving a system of linear equations of the form AX = w, where A = [aij ] ∈ Mn×n (R)   b1   is a nonsingular matrix and w =  ...  ∈ Rn . We know that this system bn −1

has a unique solution, namely A w, but inverting the matrix A may be computationally time-consuming and prone to error, so we are looking for another method. Suppose that we can write A = E − D, where E is some matrix which is easy to invert. Then if v ∈ Rn satisfies Av = w, we know that Ev = Dv + w and so v = E −1 (Dv + w). We now guess a value for v, call it v (0) . Then, using this formula, we can define new vectors v (1) , v (2) , . . . iteratively by setting v (h) = E −1 Dv (h−1) + w for each h > 0. This can be done relatively quickly since, by assumption, E −1 was relatively easy to compute and, having computed it once for the first step of the iteration, we don’t need to recompute it for subsequent steps. Our hope is that the sequence v (0) , v (1) , v (2) , . . . will in fact converge. Indeed, if this sequence does converge to some vector v then it is easy to verify that v must be the unique solution of AX = w. For example, let us assume that the diagonal entries aii of A are all nonzero, and let us choose E to be the diagonal matrix having these entries on the diagonal. Then E −1 is also a diagonal matrix having the   (0) c1  .   on the diagonal. If our initial guess is v (0) =  entries a−1 ii  ..  , (0)



then it is easy to see that for h > 0 we have v (h)

cn

 (h) c1  .   =  ..  , where (h) cn

186 (h+1)

ci


* + (h) bi − j=i aij cj for all 1 ≤ i ≤ n. This method is known = a−1 ii

as the Jacobi iteration method6 . Another possibility, again under the assumption that the diagonal entries aii of A are all nonzero, is to choose E to be the upper-triangular matrix [eij ] defined by setting

aij if i ≤ j eij = . 0 otherwise     (0) (h) c1 c1  .   .  (h)    Given an initial guess v (0) =   ..  , we see that v =  ..  for (0)

*

cn

(h)

cn

+ i−1 n (h+1) (h+1) (h) b for h > 0, where ci = a−1 − a c − a c i ij ij j j ii j=1 j=i+1 all 1 ≤ i ≤ n. This method is known as the Gauss-Seidel iteration method, since it was discovered independently by Gauss and by Jacobi’s student Philipp Ludwig von Seidel. In both of the above methods, and in other iteration methods (and there are many of these), there is no guarantee that the sequence of approximations will always converge or that, even if it does converge, it will do so rapidly. Understanding the conditions for convergence and analyzing the speed of convergence requires sophisticated techniques in numerical analysis, and indeed there are many examples of matrices for which one iteration scheme converges whereas another doesn’t, as well as various necessary and sufficient conditions for a given iteration method to converge.7 For example, a sufficient condition for the Jacobi iteration method to converge for a

6

Carl Gustav Jacob Jacobi was a 19th-century German mathematician, who worked mostly in analysis and applied mathematics. His work in astronomy led him to solve large systems of linear equations, and his papers on determinants helped make them well-known.

7

The convergence and accuracy of the Gauss-Seidel iteration method was studied in detail by the Russian mathematician and engineer Alexander Ivanovich Nekrasov at the beginning of the twentieth century, long before the use of electronic computers.


187

matrix A = [aij ] is that, j=i |aij | < |aii | for all 1 ≤ i ≤ n. As a rule of thumb, iteration methods work best for large sparse matrices – namely matrices in which a very large majority of the entries are 0 – such as those arising from the solution of systems of partial differential equations. As previously remarked, in iteration methods truncation and roundoff errors tend to cancel each other out, rather than accumulate.     7 4 2 1 Example: Let A =  −1 1 2  ∈ M3×3 (R) and let w =  2  . 4 0 1 3   1 The system of linear equations Ax = w has a unique solution  1  . If 1 we use the Jacobi iteration method beginning with the initial guess v (0) =   0  0  , we get the sequence of vectors (written to 6 digit accuracy): 0           0 1.75000 0.41667 1.04167 0.96528  0  ,  2.00000  ,  1.08333  ,  1.08333  ,  1.09722  , 0 1.33333 0.66667 0.97222 0.97222         0.95833 0.99768 0.99016 0.99614  1.02083  ,  1.02314  ,  1.01157  ,  1.00559  , 0.96759 1.01157 0.99228 0.99614     0.99816 0.99853  1.00386  ,  1.00190  , . . . 0.99814 0.99871 and if we use the Gauss-Seidel iteration method with the same initial guess, we get the sequence of vectors (written to 6 digit accuracy):           0 1.75000 1.04167 1.06944 1.01504  0  ,  −0.66667  ,  0.63889  ,  0.80093  ,  0.93672  , 0 1.33333 1.55556 1.12037 1.06636         1.00829 1.00264 1.00113 1.00040  0.97287  ,  0.99020  ,  0.99611  ,  0.99853  , 1.02109 1.00904 1.00326 1.00129     1.00016 1.00006  0.99943  ,  0.99978  , . . . 1.00049 1.00019 so we see that both methods converge, albeit quite differently.

188




   1 2 0 0 Example: Let A =  2 1 2  ∈ M3×3 (R) and let w =  −1  . 0 2 1 3   −2 The system of linear equations Ax = w has a unique solution  1  . If 1 we try to solve this system using the Gauss-Seidel method with the initial   0 guess  0  , we get the sequence of vectors 0         0 2 30 254  −1  ,  −15  ,  −127  ,  −1023  , . . . 5 33 257 2049 which clearly diverges. A more sophisticated iteration technique is, at each stage, not to replace v (i) by the computed v (i+1) but rather by a linear combination of the form rv (i+1) + (1 − r)v (i) , where 0 ≤ r is a relaxation parameter. Doing this with Jacobi iteration gives us the Jacobi overrelaxation (JOR) method, and doing it with the Gauss-Seidel method gives us the successive overrelaxation (SOR) method. The relaxation parameter r is chosen on the basis of certain properties of the matrix A. By choosing this parameter wisely, one can often achieve a considerable improvement in convergence. Example: In the beginning of this chapter we saw an example of how a nonlinear system of equations can be turned into a linear system. This can often be done in more general cases, producing large systems of linear equations of the form AX = w, where the matrix A is usually sparse and for which iteration methods are therefore appropriate. Consider, for example, the problem of finding real numbers a, b, and c such that the following conditions hold: a2 − b2 + c2 = ab + ac + 4bc = a2 + 2ab − 2bc = 2a2 − 3ab + c2 = b2 − c2 + 5ab = 2ac − 3b2 =

6 29 −7 5 5 −6

To linearize this, we begin by assigning variables to all of the terms appearing in the equations: X1 = a2 , X2 = b2 , X3 = c2 , X4 = ab, X5 = ac,


189

and X6 = bc. This then yields the system of linear equations        

1 −1 1 0 0 0 0 1 1 0 0 2 2 0 1 −3 0 1 −1 5 0 −3 0 0

  0 0 6  29 1 4     0 −2   X =  −7   5 0 0     5 0 0 2 0 −6

       

which has a unique solution X1 = 1, X2 = 4, X3 = 9, X4 = 2, X5 = 3, and X6 = 6, from which we deduce that a = 1, b = 2, and c = 3. The iterative methods we have discussed so far are all linear, in the sense that they involve only methods of linear algebra. There are, however, also families of nonlinear iterative methods, involving the calculus of functions of several variables, of which one should be aware. These include gradient (steepest-descent) methods and conjugate-direction methods. A discussion of these methods is beyond the scope of this book. Finally, another important warning. When we attempt to solve systems of linear equations on a computer, it is important to remember that the system may be very sensitive, and small changes in the entries of the coefficient matrix may lead to large changes in the solution. Such systems are said to be ill-conditioned. Applied mathematicians and others who design mathematical models often take considerable pains to avoid creating ill-conditioned systems. Example: Consider the system of linear equations        

1 0 0 0 0 0

−10 0 0 0 0 1 −10 0 0 0 0 1 −10 0 0 0 0 1 −10 0 0 0 0 1 −10 0 0 0 0 1





      X =        

   over R. This system has a unique solution, namely    

1 1 1 1 1 1

−9 −9 −9 −9 −9 1

       

     . However, if we   

alter the coefficient matrix by changing the (6, 6)-entry to

1 1.001

(which is

190


roughly equal to  101  11   2 namely   1.1   1.01 1.001

0.9990009), we will obtain a completely different solution,     .   

Since real-life computations are based, as a rule, on numbers gathered through some sort of measurement process, which is as a matter of course not completely accurate and certainly beyond our control, it is extremely important to know how sensitive the system is to possible small variations in the values of the entries. The numerical analysis of matrices deals extensively with this issue, and here we can only present a simplistic measure of this sensitivity for nonsingular square matrices over R. To any ma∈ Mn×n(R), we will assign the number θ(A) defined by trix A = [aij ] n |aij | . The number θ(A)θ(A−1 ) is the condition θ(A) = max 1≤j≤n

i=1

number8 of the matrix A. Note that A has the same condition number as A−1 and as cA, for any 0 = c ∈ R. The condition number can be written in the form g × 10t . where 0.1 ≤ g < 1. If t > 0 then, as a rule of thumb, one can expect that the solution of a system of linear equations AX = w will have t significant digits fewer than that of the entries of A. Thus, if A is the matrix in the previous example, then θ(A) = 11. Moreover,  A−1

   =   

1 0 0 0 0 0

10 1 0 0 0 0

100 10 1 0 0 0

1000 100 10 1 0 0

10000 1000 100 10 1 0

100000 10000 1000 100 10 1

       

8 Condition numbers were introduced by John von Neumann, one of the great mathematical geniuses of the 20th century, who contributed to practically all branches of mathematics – pure and applied. Von Neumann was a major force in the the introduction of digital computers after World War II and the development of numerical methods for them.


191

and so θ(A−1 ) = 11, 1111. Therefore θ(A)θ(A−1 ) is roughly 12 × 107 , and so we cannot, as we have seen, expect any accuracy in our solution, if we assume our data is only good to 6-digit accuracy. ! 888445 887112 Similarly, Nievergelt’s matrix , which we have al887112 885871 ready encountered, has condition number roughly equal to 0.39 × 105 . Of course, computing the condition number of a given matrix may also be a problem, since it involves calculating A−1 . Fortunately, there are many fairly-efficient condition number estimators, algorithms that give a good estimate of the condition number of a matrix with relatively low computational overhead.

Exercises 

−3 4 Exercise 522 Are the matrices  −2 −4 5 2 in M3×3 (R) row equivalent?  1 2 3 Exercise 523 Bring the matrix  1 2 4 2 3 1 row echelon form.

  1 1 −6  and  0 7 0

0 1 0

 1 1  0

 4 3  ∈ M3×4 (R) to reduced 4 

 1 2 1 0 Exercise 524 Let F = GF (5). Bring the matrix  2 3 1 1  ∈ 1 2 4 0 M3×4 (F ) to reduced row echelon form.

Exercise 525 Solve the system of linear equations (3 − i)X1 + (2 − i)X2 + (4 + 2i)X3 (4 + 3i)X1 − (5 + i)X2 + (1 + i)X3 (2 − 3i)X1 + (1 − i)X2 + (2 + 4i)X3 over C. Exercise 526 Solve the system of linear equations X1 + 2X2 + 4X3 5X1 + X2 + 2X3 3X1 − X2 + X3 over R.

=

31

= =

29 10

= =

2 + 6i 2 + 2i

=

5i

192


Exercise 527 Solve the system of linear equations 3X1 + 4X2 + 10X3 2X1 + 2X2 + 2X3 X1 + X2 + 5X3

= =

1 0

=

1

over GF (11). Exercise 528 Find all  1  2   3 4

solutions to the system    2 3 4 5 X1  X2   1 1 2 3  =  2 1 2   X3   1 X4 3 2 1 −5

   

over R. Exercise 529 Find all solutions to the   1 2 3 4 5  2 1 2 3 4     2 2 1 2 3     2 2 2 1 2  2 2 2 2 1

system   X1  X2     X3  =   X4   X5

13 10 11 6 3

     

over R. Exercise 530 Find all solutions to the system       X 1 1 1 1 1  1   1 1 1 0   X2  =  0   X3  1 0 0 1 1 X4 over GF (2). Exercise 531 Find all solutions  1 3 2  2 −1 3   3 −5 4 1 17 4

to the system      0 X 1  0     X2  =    0   X3 0

over R. Exercise 532 Find a real number a so that the system of linear equations 2X1 − X2 + X3 + X4 X1 + 2X2 − X3 + 4X4 X1 + 7X2 − 4X3 + 11X4 has a solution over R.

= 1 = 2 = a


193

Exercise 533 Find all real numbers c such that the system of equations X1 + X 2 − X 3 X1 + cX2 + 3X3 2X1 + 3X2 + cX3

= =

1 2

=

3

has a unique solution over R; find those real numbers c for which it has infinitely-many solutions over R; find those real numbers c for which it has no solution over R. Exercise 534 Solve the system of linear equations X1 + 2X2 + X3 X 1 + X2 + X3

= =

1 0

over GF (3). Exercise 535 Solve the system of linear equations √ √ X1 + ( 2)X2 + ( 2)X3 = 3 √ √ X1 + (1 + 2)X2 + X3 = 3 + 2 √ √ X1 + X2 − ( 2)X3 = 4 + 2 √ over Q( 2). Exercise 536 Solve the system of linear equations 4X1 − 3X2 2X1 − X2 + 2X3 3X1 + 2X3

= 3 = 1 = 4

over GF (5). Exercise 537 Solve the system of linear equations 4X1 + 6X2 + 2X3 X1 − aX2 − 2X3 7X1 + 3X2 + (a − 5)X3

=

8

= =

−5 7

over R, for various values of the real number a. Exercise 538 For a given real number a, solve the system aX1 + X2 + X3 X1 + aX2 + X3 X1 + X2 + aX3 over R.

= =

1 1

=

1

194


Exercise 539 For a ∈ R does the system of linear equations aX1 + X2 + 2X3 X1 − X2 + aX3 X 1 + X2 + X3

=

0

= =

1 1

have a unique solution in R? Exercise 540 Let a be an element of a field F. Find the set of all solutions to the system of linear equations X1 + X2 + aX3 X1 + aX2 − X3 X 1 + X2 − X3

= = =

a 1 1

over F. Exercise 541 For which a ∈ Q does the system of linear equations X1 + 3X2 − 2X3 3X1 + 9X2 − 2X3 2X1 + 6X2 + X3

= =

2 2

=

a

have a unique solution in Q? Exercise 542 Find real numbers a, b, c, and d such that the points (1, 2), (−1, 6), (−2, 38), and (2, 6) all lie on the curve y = ax4 + bx3 + cx2 + d in the euclidean plane. Exercise 543 Find a polynomial p(X) = a2 X 2 + a1 X + a0 ∈ R[X] satisfying p(1) = −1, p(−1) = 9, and p(2) = −3. Exercise 544 Find a polynomial p(X) = a3 X 3 +a2 X 2 +a1 X +a0 ∈ R[X] satisfying p(0) = 2, p(2) = 6, p(4) = 3, and p(6) = −5. Exercise 545 Let F = GF (13). Find a homogeneous system of linear equations over F satisfying the condition that its solution space equals       2 8 7       1   3   6           ,  10  ,  2  . 9 F          7   5   11         4 12 7 Exercise 546 Let F be a field. Let b ∈ F and let ! a11 a12 a13 ∈ M2×3 (F ) A= a21 a22 a23 be a matrix satisfying the condition that the sum of the entries in each row and each column of A equals b. Show that b = 0.


195

Exercise 547 Let p(X) = X 5 − 7X 3 + 12 ∈ Q[X]. Find a polynomial q(X) ∈ Q[X] of degree at most 3 satisfying p(a) = q(a) for all a ∈ {0, 1, 2, 3}.   1 0 0 0 0 0  0 0 0 1 1 0     1 1 1 1 0 0     Exercise 548 Find the rank of the matrix   0 1 1 1 0 0  ∈  0 1 1 0 1 0     1 0 0 1 1 0  1 1 1 0 1 0 M7×6 (GF (2)). Exercise 549 Find the rank of the matrix  1 −1 2 3 4  2 1 −1 2 0   −1 2 1 1 3   1 5 −8 −5 −12 3 −7 8 9 13 Exercise 550 Find the  1  1   0   0 0

    ∈ M5×5 (R).  

rank of the matrix  0 1 0 0 1 0 0 0   1 1 0 0   ∈ M5×5 (R). 0 1 −1 0  1 0 1 1

Exercise 551 Let F = GF (2).  1 1  0 1 1 0

Find the rank of the matrix  0 1  ∈ M3×3 (F ). 1

Exercise 552 Let F = GF (5). Find the rank of the matrix   1 2 3 4 a  4 3 a 1 2    ∈ M4×5 (F )  a 1 2 3 4  2 3a 2 4a 1 for various values of a ∈ F. Exercise 553 Do there exist a lower-triangular matrix L and an uppertriangular matrix U in M3×3 (Q) satisfying the condition LU =   1 −1 2  2 −1 3  ? 0 1 8

196


Exercise 554 Let F = GF (5). For which values of a ∈ F do there exist a lower-triangular matrix L and an upper-triangular matrix U in   1 1 a M3×3 (F ) satisfying the condition that LU =  4 1 0  ? a 1 4 Exercise 555 Find the LU-decomposition of the matrix   4 2 3 4  2 0 2 2   A=  3 4 −4 5  ∈ M4×4 (R). −1 0 2 3 Exercise 556 Let A ∈ Mn×n (R) be a tridiagonal matrix all diagonal entries of which are nonzero. Can we write A = LU, where L is a lower-triangular matrix and U is an upper-triangular matrix, both of which are also tridiagonal? Exercise 557 Let F be a field and let a, b, c ∈ F . Find the rank of the   1 1 1 matrix  b + c c + a a + b  ∈ M3×3 (F ). bc ca ab Exercise 558 Let F be a field and let a, b, c, d ∈   a c c the matrix  d a + b c  ∈ M3×3 (F ). d d b  3 1  a 4 Exercise 559 Find the rank of the matrix   1 7 2 2 for various values of the real number a. Exercise 560 Find the rank of  a −1  −1 a 10 −6

F. Find the rank of

 1 4 10 1   ∈ M4×4 (R) 17 3  4 3

the matrix  2 1 5 2  ∈ M3×4 (Q) 1 1

for various values of the rational number a. Exercise 561 Find the set of all real numbers a such that the rank of   a 1 1 the matrix  −1 −1 −1  ∈ M3×3 (R) equals 2. 1 1 a


197

Exercise 562 Let n be a positive integer and, for each A ∈ Mn×n (R), let r(A) be the rank of A. Define a relation on Mn×n (R) by setting B A if and only if r(A − B) = r(A) − r(B). Is this a partial order relation? Exercise 563 Let F be a subfield of a field K. Let k and n be positive integers and let A ∈ Mk×n (F ) be a matrix having rank r. If we now think of A as an element of Mk×n (K), is its rank necessarily still equal to r? Exercise 564 Find an integer  1 7  4 4   3 1 2a 8

a such that the rank of the matrix  17 3 8 6   ∈ M4×4 (Q) 1 4  20 2

is minimal. Exercise 565 Let F be a field and let k and n be positive integers. For a matrix A ∈ Mk×n (F ) having rank h, show that there exist matrices B ∈ Mk×h (F ) and C ∈ Mh×n (F ) such that A = BC. Exercise 566 Let k and n be positive integers and let F be a field. For matrices A, B ∈ Mk×n (F ), show that the rank of A + B is no more than the sum of the ranks of A and of B. Exercise 567 Let k and n be positive integers and let F be a field. Let A, B ∈ Mk×n (F ) be matrices satisfying the condition that he row space of A and the row space of B are disjoint. Does it follow from this that the rank of A + B equals the sum of the rank of A and the rank of B? Exercise 568 Find bases for the row space and column space of the matrix   1 2 −3 −7 −2  −1 −2 1 1 0  ∈ M3×5 (R). 1 2 0 2 1 P, Q ∈ M3×3 (R) satisfying    3 1 0 0 1 Q =  0 1 0 . 4 0 0 0  1 Exercise 570 Write the rows of the matrix A =  i − 1 0 M3×3 (C) as linear combinations of the rows of AT . Exercise 569 Find matrices  1 2 P  2 −2 3 0

 2 0 2 i  ∈ 2 −i

198


   Exercise 571 Calculate    Exercise B A= D matrix in A equals

1 0 0 0 0

2 1 0 0 0

3 2 1 0 0

4 3 2 1 0

5 4 3 2 1

−1     

∈ M5×5 (R).

572 !Let k and n be positive integers and let F be a field. Let C be a matrix in Mk×n (F ), where B is a nonsingular E Mr×r (F ) for some 1 ≤ r < min{k, n}. Show that the rank of r if and only of DB −1 C = E.

Exercise 573 Let F be a field and let a, b, c be distinct elements of F. Furthermore, let d, e, f be distinct elements of F. What is the rank of   1 a d ad the matrix  1 b e be  ∈ M3×4 (F )? 1 c f cf Exercise 574 Let k and n be positive integers and let F be a field. Let A ∈ Mk×n (F ) and let w ∈ F k be such that the system of linear equations AX = w has a nonempty set of solutions and that all of these solutions satisfy the condition that the hth entry in them is some fixed scalar c. What can we deduce about the columns of the matrix A? Exercise 575 Let n be a positive integer and let F be a field. Let O = A ∈ Mn×n (F ). Show that there exists a nonnegative integer k such that the rank of Ah equals the rank of Ak for all h > k.   1 −1 1 Exercise 576 Let A =  −1 −1 1  ∈ M3×3 (R). Find the condition 1 1 1 number of A. Exercise 577 Let a be a positive real number. It is necessarily true that   a 1 a 0 −1  ∈ M3×3 (R) is greater the condition number of A =  0 a −1 a than 2a + 1? Exercise 578 Find a positive real number a for which the condition   1 1 0 number of A =  0 a a  ∈ M3×3 (R) is maximal. 1 1 1 Exercise 579 Does there exist a system AX = w of linear equations in n unknowns (for some positive integer n) over R having precisely 35 distinct solutions?

11 Determinants

Let F be a field and let n be a positive integer. We would like to find a function from Mn×n (F ) to F which will serve as an oracle of singularity, namely a function that will assign a value of 0 to singular matrices and a value other than 0 to nonsingular matrices. Indeed, let F be a field and let n be a positive integer. A function δ n : Mn×n (F ) → F is a determinant function if and only if it satisfies the following conditions: (1) δ n (I) = 1; (2) δ n (A) = 0 if A is a matrix having a row all of the entries of which are 0; (3) δ n (Eij A) = −δ n (A) for all 1 ≤ i = j ≤ n; (4) δ n (Eij;c A) = δ n (A) for all 1 ≤ i = j ≤ n and all c ∈ F ; (5) δ n (Ei;c A) = cδ n (A) for all 1 ≤ i ≤ n and all 0 = c ∈ F. In particular, we note that for each 1 ≤ i = j ≤ n and all c ∈ F T T ), δ n (Eij;c ) = 1 = δ n (Eij;c ), and we have δ n (Eij ) = −1 = δ n (Eij T δ n (Ei;c ) = c = δ n (Ei;c ). We have yet to show that such functions exist for all values of n, but certainly they exist for a few small ones. Example: For n = 1, the function δ 1 : [a] → !a is a determinant a11 a12 function. For n = 2, the function δ 2 : → a11 a22 − a12 a21 a21 a22 is a determinant function. 199

200

11. Determinants

As an immediate consequence of parts (1) and (5) of the definition, we see (F ) → that if A = [aij ] ∈ Mn×n (F ) is a diagonal matrix n and if δ n : M n×n n F is a determinant function, then δ n (A) = i=1 aii δ n (I) = i=1 aii . We now want to show that for each positive integer n there exists determinant function δ n : Mn×n (F ) → F, and indeed that this function is unique. We will first establish the uniqueness of these functions and check some of their properties, holding off on existence until later in this chapter. (11.1) Proposition: Let F be a field. For each positive integer n there exists at most one determinant function δ n : Mn×n (F ) → F. Proof: Let us assume that δ n : Mn×n (F ) → F and η n : Mn×n (F ) → F are determinant functions and let β = η n − δ n . Then the function β satisfies the following conditions: (1) β(I) = 0; (2) β(A) = 0 if A is a matrix having a row all of the entries of which are 0; (3) β(Eij A) = −β(A) for all 1 ≤ i = j ≤ n; (4) β(Eij;c A) = β(A) for all 1 ≤ i = j ≤ n and all c ∈ F ; (5) β(Ei;c A) = cβ(A) for all 1 ≤ i ≤ n and all 0 = c ∈ F. In particular, if A ∈ Mn×n (F ) and E is an elementary matrix, then β(A) and β(EA) are either both equal to O or both of them are different from O. But for any matrix A we know that there exist elementary matrices E1 , . . . , Et in Mn×n (F ) such that either E1 · . . . · Et A = I or E1 · . . . · Et A is a matrix having at least one row all of the entries of which equal 0. Therefore β(A) = 0 for every A ∈ Mn×n (F ). Thus β is the zero-function, and so δ n = η n . (11.2) Proposition: Let F be a field and let δ n : Mn×n (F ) → F be a determinant function. Then δ n (A) = 0 if and only if A is nonsingular. Proof: If A is nonsingular, there exist elementary matrices E1 , . . . , Et in Mn×n (F ) such that E1 · . . . · Et A = I, and so, by the definition of the determinant function, δ n (A) = cδ n (I) = c, where 0 = c ∈ F, and so δ n (A) = 0. Now assume that δ n (A) = 0 and that A is singular. Then there exist elementary matrices E1 , . . . , Et in Mn×n (F ) such that E1 · . . . · Et A is a matrix having at least one row all of the entries of which equal 0. But then, for some 0 = c ∈ F, we have 0 = δ n (A) = cδ n (E1 · . . . · Et A) = c0 = 0, which is a contradiction, proving that A must be nonsingular.

11. Determinants

201

Thus we see that the determinant function, to the extent it exists, is the oracle we are seeking.

! !a + bi −c + di Example: The subset , of C2 is linearly c + di a − bi ! a + bi −c + di dependent if and only if A = ∈ M2×2 (C) is singular. c + di a − bi ! a11 a12 → a11 a22 − a12 a21 is a We have already noted that δ 2 : a21 a22 determinant function, and so this happens if and only if δ 2 (A) = a2 + b2 + c2 + d2 = 0, i.e. if and only if a = b = c = d = 0. (11.3) Proposition: Let F be a field and let δ n : Mn×n (F ) → F be a determinant function. If A is a matrix in Mn×n (F ) having two identical rows then δ n (A) = 0. Proof: Suppose that rows h and k of A are identical. First assume that the characteristic of F is other than 2. Then A = Ehk (A) and so δ n (A) = δ n (Ehk A) = −δ n (A), which implies that δ n (A) = 0. If the characteristic of F equals 2 then δ n (A) = δ n (Ehk;1 A), and Ehk;1 A is a matrix having a row in which the entries of one row are all 0. Therefore, by Proposition 11.2, δ n (A) = 0. (11.4) Proposition: Let F be a field and let δ n : Mn×n (F ) → F be a determinant function. If A, B ∈ Mn×n (F ) then (1) δ n (AB) = δ n (A)δ n (B); (2) δ n (AB) = δ n (BA). Proof: (1) By Proposition 9.1, we know that AB is nonsingular if and only if both A and B are nonsingular. Therefore δ n (A) = 0 or δ n (B) = 0 if and only if δ n (AB) = 0. If δ n (A) = 0 = δ n (B) then there exist elementary matrices E1 , . . . , Et , G1 , . . . , Gs in Mn×n (F ) such that B = E1 · . . . · Et I and A = G1 · . . . · Gs I and so AB = G1 · . . . · Gs E1 · . . . · Et I, which implies that δ n (AB) = δ n (A)δ n (B) from the definition of a determinant function. (2) This is an immediate consequence of (1), since δ n (A)δ n (B) = δ n (B)δ n (A) in F . (11.5) Proposition: Let F be a field and let δ n : Mn×n (F ) → F be a determinant function. If A ∈ Mn×n (F ) is nonsingular then δ n (A−1 ) = δ n (A)−1 . Proof: By Proposition 11.4, we see that δ n (A−1 )δ n (A) = δ n (A−1 A) = δ n (I) = 1 and from this the result follows immediately.

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(11.6) Proposition: Let F be a field and let δ n : Mn×n (F ) → F be a determinant function. If A ∈ Mn×n (F ) then: (1) δ n (AEij ) = −δ n (A) for all 1 ≤ i = j ≤ n; (2) δ n (AEij;c ) = δ n (A) for all 1 ≤ i = j ≤ n and all c ∈ F ; (3) δ n (AEi;c ) = cδ n (A) for all 1 ≤ i ≤ n and all 0 = c ∈ F. Proof: This is a direct consequence of the definition of the determinant function and Proposition 11.4(2). (11.7) Proposition: Let F be a field and let δ n : Mn×n (F ) → F be a determinant function. If A ∈ Mn×n (F ) then δ n (A) = δ n (AT ). Proof: If A is singular then so is AT and so δ n (A) = 0 = δ n (AT ). If A is nonsingular then there exist elementary matrices E1 , . . . , Et in Mn×n (F ) such that E1 · . . . · Et A = I = I T = AT EtT · . . . · E1T . By our remarks in Chapter 9 concerning the transposes of elementary matrices, and by the remarks at the beginning of this chapter, we see that δ n (A) = δ n (E1 · . . . · Et A) = δ n (AT EtT · . . . · E1T ) = δ n (AT ) and so δ n (A) = δ n (AT ). Of course, at this stage we do not know that determinant functions δ n : Mn×n (F ) → F even exist for the case n > 2 and so we now have to construct them. Let us denote the set of all permutations of the set {1, . . . n} by Sn . We note that any π ∈ Sn is a bijective function from {1, . . . n} to itself and so there exists a function π −1 ∈ Sn satisfying the condition that ππ −1 and π −1 π are equal to the identity function i → i. We also note that if π, π ∈ Sn then ππ ∈ Sn . (11.8) Proposition: If n is a positive integer then the number of elements of Sn equals n!. Proof: Suppose we wanted to construct an arbitrary element π of Sn . There are n possibilities for selecting π(1). Once we have done that, there are n − 1 ways of selecting π(2), then n − 2 ways of selecting π(3), etc. Thus, the total number of ways in which we can define π is n(n − 1) · . . . · 1 = n!. Now let π ∈ Sn and let 1 ≤ i < j ≤ n. The pair (i, j) is called an inversion with respect to π if and only if π(i) > π(j). That is to say, (i, j) is an inversion with respect to π if and only if i−j < 0. π(i) − π(j)

11. Determinants

203

We will denote the number of distinct inversions with respect to π by h(π), and define the signum of π to be sgn(π) = (−1)h(π) . Thus  if there are an even number of inversions    1 with respect to π sgn(π) = . if there are an odd number of inversions   −1  with respect to π It is easy to check that sgn(π) = sgn(π −1 ) for all π ∈ Sn . If sgn(π) = 1, the permutation π is even; if sgn(π) = −1, the permutation π is odd. Example: Let π ∈ S4 be defined by 1 → 3, 2 → 4, 3 → 2, and 4 → 1. Then if we consider all possible pairs (i, j) with 1 ≤ i < j ≤ 4 we get (i, j) (π(i), π(j)) inversion? (1,2) (3,4) no (3,2) yes (1,3) (3,1) yes (1,4) (4,2) yes (2,3) (4,1) yes (2,4) (2,1) yes (3,4) and so we see that sgn(π) = −1. Now let n be a positive integer and let (K, •) be an associative and commutative unital F -algebra. Let A = [aij ] ∈ Mn×n (K). We then define the function A → |A| from Mn×n (K) to K by setting |A| = sgn(π)aπ(1),1 • aπ(2),2 • . . . • aπ(n),n . π∈Sn

Note that, by the commutativity of K, if τ = π −1 then aπ(1),1 • aπ(2),2 • . . . • aπ(n),n = a1,τ (1) • a2,τ (2) • . . . • an,τ (n) and so |A| = τ ∈Sn sgn(τ )a1,τ (1) • a2,τ (2) • . . . • an,τ (n) . Thus we see immediately that |A| = |AT | for every A ∈ Mn×n (K). If K = C then, since c + d = c + d and cd = cd, we also see that for A = [aij ] we have |A| = |A|. Defining this function for an arbitrary commutative and associative unital F -algebra is important for us, as we will need it in the case that K = F [X], where F is a field. Example: If A = [aij ] ∈ M3×3 (K), for an associative and commutative unital F -algebra (K, •), then |A|

=

a11 • a22 • a33 + a12 • a23 • a31 + a13 • a21 • a32 −a11 • a23 • a32 − a13 • a22 • a31 − a12 • a21 • a33 .

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(11.9) Proposition: Let F be a field, let (K, •) be an associative and commutative unital F -algebra, and let A = [aij ] ∈ Mn×n (K). Pick 1 ≤ h ≤ n and write ahj = bhj + chj in K for all 1 ≤ j ≤ n. For all 1 ≤ i ≤ n satisfying i = h, set bij = cij = aij . Set B = [bij ] and C = [cij ], matrices in Mn×n (K). Then |A| = |B| + |C|. Proof: From the definition of |A|, we have |A| = sgn(π)a1,π(1) • . . . • ah,π(h) • . . . • an,π(n) π∈Sn

=

) ( sgn(π)a1,π(1) • . . . • bh,π(h) + ch,π(m) • . . . • an,π(n)

π∈Sn

=

sgn(π)a1,π(1) • . . . • bh,π(h) • . . . • an,π(n)

π∈Sn

+

sgn(π)a1,π(1) • . . . • ch,π(h) • . . . • an,π(n)

π∈Sn

= as required.

|B| + |C|,

We are now ready to prove that determinant functions in fact always exist. (11.10) Proposition: For an integer n > 1 and a field F , the function Mn×n (F ) → F defined by A → |A| is a determinant function. Proof: In order to simplify our notation, we will make the following temporary convention: if π ∈ Sn and if A = [aij ] ∈ Mn×n (F ), we will write u(π, A) = sgn(π)a1,π(1) · . . . · an,π(n) . Now let us check the five conditions of a determinant function. (1) Clearly u(π, I) equals 1 if π is the identity permutation and 0 otherwise, and so |I| = 1. (2) Let A be a matrix one of the rows of which has all of its entries equal to 0. Since a factor from each row appears in every term u(π, A), we conclude that all of these are equal to 0 and hence |A| = 0. (3) Let A be a matrix and let B = Eij A. Let ρ ∈ Sn be the permutation which interchanges i and j and leaves all of the other numbers between 1 and n fixed. Then sgn(πρ) = sgn(π) for all π ∈ Sn and so for each π ∈ Sn we have −u(π, A) = u(πρ, A) = u(π, B). This implies that |B| = −|A|. (4) Let A be a matrix and let B = Eij;c A. Then B = [bht ], where bht = aht when h = j and 1 ≤ t ≤ n, and where bjt = ajt + cait for all

11. Determinants

205

1 ≤ t ≤ n. By Proposition 11.9, we have |B| = |A| + |C|, where C is the matrix all of the rows of which except the jth are identical with those of A, and where in the jth row we have cjt = cait for all 1 ≤ t ≤ n. Then |C| = c|D| where D is a matrix in which two rows, the ith and the jth, are equal. If the characteristic of F is other than 2, then D = Eij D and so, by (3), we get |D| = −|D|, and so we get |C| = c|D| = 0 and we have |A| = |B|, which is what we want. Therefore let us assume that the characteristic of F equals 2. Let ρ ∈ Sn be the permutation which interchanges i and j and leaves all other numbers between 1 and n fixed. Let H be the set of all even permutations in Sn and let K be the set of all odd permutations. The function from H to K defined by π → ρπ is bijective since ρπ 1 = ρπ 2 implies that π 1 = ρ−1 ρπ 1 = ρ−1 ρπ 2 = π 2 . Moreover, since the characteristic of F is 2 and since u(π, D) = u(ρπ, D) for all π ∈ H, we see that u(π, D) + u(ρπ, D) = 0 for all π ∈ H. Therefore |D| = π∈H [u(π, D) + u(ρπ, D)] = 0 and this implies, again, that |C| = 0 and so |A| = |B|. (5) It is clear from the definition of |A| and if B = Ei;c A then |B| = c|A|. Thus, in summary, we see that if F is a field and if n is a positive integer, then there exists a unique determinant function Mn×n (F ) → F, namely A → |A|. We call the scalar |A| the determinant1 of the matrix A. Example: Let n > 1 be an integer. If c1 , . . . cn are distinct elements of a field F and if A = [aij ] ∈ Mn×n (F ) is the Vandermonde matrix for all 1 ≤ i, j ≤ n, then it is easy to verify that definedby aij = cj−1 i |A| = (cj − ci ) = 0. i<j

Example: As a consequence of Proposition 11.7, we note that if n > 0 is odd and if A ∈ Mn×n (F ) is a skew-symmetric matrix then |A| =

1

Determinants were first used in the work of the 17th-century German mathematician, philosopher, and diplomat Gottfried von Leibnitz, who developed calculus along with Sir Isaac Newton. The common properties of determinants were first studied by 19th-century German mathematician Heinrich Scherk, and the first systematic analysis of the theory of determinants was done by the 19th-century French mathematician Augustin-Louis Cauchy, relying on the work of many mathematicians who preceded him. His work was continued by Cayley and Sylvester.

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11. Determinants

T A = |−A| = − |A| and so |A| = 0. Therefore, by Proposition 11.2, A is singular. If n is even, then one can use the definition of |A| to show that |A| = b2 for some b which is a sum of products of the aij . Thus, for example, 0 a13 a14 a12 −a12 0 a23 a24 2 = [a12 a34 − a13 a24 + a14 a23 ] . −a13 −a23 0 a34 −a14 −a24 −a34 0 This number b is called the Pfaffian2 of the matrix A. Pfaffians arise naturally in combinatorics, differential geometry and other areas of mathematics. We now give two examples of why it was worthwhile to define |A| for matrices A with entries in an associative and commutative unital F algebra, and not just a field. Example: Let V be a vector space of finite dimension n over a field F and let B = {v1 , . . . , vk } be a linearly-independent subset of V. Let y1 , . . . , yk be a list of vectors in V. We claim that there are at most finitely-many elements a of F satisfying the condition that the list v1 + ay1 , . . . , vk + ayk is linearly dependent. To establish this claim, we will consider determinants of matrices over F [X]. Indeed, extend B to a basis D= {v1 , . . . , vn } of V. Then, for each 1 ≤ i ≤ k, we can n write yi = j=1 cij wj . For each 1 ≤ i, j ≤ k, define the polynomial pij (X) ∈ F [X] by setting

cii X + 1 if i = j pij (X) = otherwise cij X and consider the matrix B = [pij (X)] ∈ Mk×k (F [X]). Then |B| is a polynomial q(X) in F [X], which is not the 0-polynomial since q(0) = 1. Moreover, for any a ∈ F, we see that q(a) = 0 whenever the list v1 + ay1 , . . . , vk + ayk

2 Pfaffians were first defined by Cayley, and named in honor of Johann Pfaff, an 18th-century German mathematician whose most famous doctoral student was Gauss.

11. Determinants

207

is linearly dependent. Since a polynomial can have only finitely-many distinct roots, this can happen only for finitely-many values of a. Example: Let n > 1 be an integer and let U be an open interval of real numbers. Let K be the set of all functions in RU which are differentiable at least n − 1 times. Then K is an associative and commutative unital R-algebra which is not entire, let alone a field. We will denote the derivative of a function f ∈ K by Df and, if h > 1, we will denote the hth derivative of f by Dh f. Given f1 , . . . , fn ∈ K, the function f2 (t) ... fn (t) f1 (t) (Df1 )(t) (Df )(t) . . . (Df )(t) 2 n W (f1 , . . . , fn ) : t → .. .. .. . . . (Dn−1 f1 )(t) (Dn−1 f2 )(t) . . . (Dn−1 fn )(t) is called the Wronskian3 of f1 , . . . , fn . One can show that if we have W (f1 , . . . , fn )(t) = 0 for some t ∈ U then the subset {f1 , . . . , fn } of K is linearly independent over R. The converse is false. To see this, 3 let U be an open interval containing the origin, let f1 : t → t , and 3 let f2 : t → t . Then {f1 .f2 } is linearly independent over R, but W (f1 , f2 )(t) = 0 for any t ∈ U. Example: Let n be a positive integer equal to 2 or divisible by 4. A matrix A = [aij ] ∈ Mn×n (C) with |aij | ≤ 1 for all 1 ≤ i, j ≤ n having maximal possible determinant (in absolute value) is known as a Hadamard matrix (though in fact such matrices were studied by Sylvester a generation before Hadamard considered them). For such a matrix, we have |A| = nn/2 , and the entries of A are all ±1. Indeed, a matrix A is a Hadamard matrix precisely when all of its entries are ±1 and AAT = nI.     −1 1 1 1 1 1 1 1  1 −1  1 1  1 −1   and  1 −1  are Hadamard Thus,   1   1 −1 1 1 1 −1 −1  1 1 1 −1 1 −1 −1 1

3

The insight of Josef Wronski, a 19th-century Polish mathematician living in France, was obscured by his decidedly eccentric philosophical ideas and style of writing, and was recognized only after his death. The notion of a determinant of functions was first used by Jacobi.

208

11. Determinants

matrices. Indeed, for each t ≥ 1, there exists a Hadamard matrix Ht ! 1 1 t t of size 2 × 2 , defined recursively by setting H1 = and 1 −1 ! Ht−1 Ht−1 for each t > 1. Ht = Ht−1 −Ht−1 We also note immediately that if A is a Hadamard matrix so are AT and −A. Hadamard matrices have important applications in algebraic coding theory, especially in defining the error-correcting ReedMuller codes. Needless to say, the determinants of Hadamard matrices get very big very quickly. If A is a 16 × 16 Hadamard matrix, then |A| = 4, 294, 967, 296 and if B is a 32 × 32 Hadamard matrix, then |B| = 1, 208, 925, 819, 614, 629, 174, 706, 176. We still are faced with the problem of actually computing the determinant of an n × n matrix A, especially when n is large. If we work using the definition, we see that we must add n! summands, each of which requires n − 1 multiplications. The total number of arithmetic operations need is therefore (n − 1)n! + (n! − 1) = n(n!) − 1, which is a huge number even if n is relatively small. For example, if we are using a computer capable of performing a billion arithmetic operations per second, it would take us 12, 200, 000, 000 years of nonstop computation to compute the determinant of a 25 × 25 matrix, based on the definition. Thus we must find better methods of computing determinants, a task which became a high priority for many nineteenth-century mathematicians. Example: Let A = [aij ] ∈ Mn×n (F ) be a matrix in which a11 = 0. Then Chi` o, Dodgson4 , and others showed that |A| = a2−n 11 |B|, where B ∈ M(n−1)×(n−1) (F ) is the matrix obtained from A by erasing the a11 a1j . first row and first column and replacing each other aij by ai1 aij

4

During the 19th century, matrix theory and the theory of determinants attracted many gifted mathematicians and mathematical amateurs. Felice Chi` o was a 19th-century Italian mathematician and physicist. On the other hand, Rev. Charles Lutwidge Dodgson was an amateur who is better known by his pen name Lewis Carroll, the author of Alice in Wonderland. Dodgson published several works on mathematics under his own name.

11. Determinants

209

Thus, for example,

1 8 1 3

2 7 8 6

3 6 2 4

4 5 7 5

= =

1 8

2 7

1 3 8 6

1 4 8 5

1 1

2 8

1 3 1 2

1 4 1 7

1 3

2 6

1 3 3 4 −9 −18 −27 6 −1 3 0 −5 −7 = −144.

1 4 3 5

This method can, of course, be iterated. Let A = [aij ] ∈ Mn×n (K), where K is an associative and commutative unital F -algebra. For each 1 ≤ i, j ≤ n, we define the minor of the entry aij of A to be |Aij |, where Aij ∈ M(n−1)×(n−1) (K) is the matrix obtained from A by erasing the ith row and the jth column. 

4 Example: If A =  2 7 ! 4 1 . 7 4

 1 9  , then A13 = 4

3 8 3

2 8 7 3

! and A22 =

(11.11) Proposition: Let F be a field, let (K, •) be an associative and commutative unital F -algebra. If nn is a positive integer, and A = [aij ] ∈ Mn×n (K), then |A| = j=1 (−1)t+j atj • |Atj | for each 1 ≤ t ≤ n.

Proof: In order to simplify our notation, let det(y1 , . . . , yn ) denote the determinant of the matrix the rows of which are y1 , . . . , yn . We will first prove the theorem case t = 1. That is to say, we must show n for the1+j (−1) a • |A1j |. For each 1 ≤ h ≤ n, let that |A| equals j=1 ) ( 1j d1 . . . dn defined by vh ∈ M1×n (K) be the matrix

di =

1 if i = h . 0 otherwise

210

11. Determinants

Then the ith row of A can be written as wi = |A| =

n j=1

aij vj . and so

  n a1j vj , w2 , . . . , wn  det(w1 , . . . , wn ) = det  j=1

=

n

a1j • det(vj , w2 , , . . . , wn ).

j=1

Thus we will prove the desired result if we can show that det(vj , w2 , , . . . , wn ) = (−1)1+j |A1j | for each 1 ≤ j ≤ n. Denote the matrix the rows of which are vj , w2 , , . . . , wn by B = [bih ], where  if i = 1 and h = j  1 0 if i = 1 and h = j . bih =  aih if i > 1. For 1 ≤ j ≤ n, set G1j = {π ∈ Sn | π(1) = j} . Suppose that j = 1. Then, in particular, there is a bijective correspondence between G11 and the set of all permutations of {2, . . . n} which does not affect the signum of the permutation since if π ∈ G11 then 1 does not appear in any inversion of π. Since b11 = 1 and b1h = 0 if h > 1, we thus have sgn(π)b1,π(1) • . . . • bn,π(n) |B| = π∈Sn

=

sgn(π)b1,π(1) • . . . • bn,π(n)

π∈G11

=

sgn(π)b2,π(2) • . . . • bn,π(n) = |A11 |

π∈G11

and so we have shown, as desired, that |B| = (−1)1+1 |A11 |. If j > 1 put column j of B in the position of the first column and shift columns 1 to j − 1 of B to the right by one column position. This involves j − 1 column interchanges, and we have 1 0 ... 0 a2j a21 . . . a2n j+1 |A1j | . det(vj , w2 , . . . , wn ) = (−1)j−1 . .. .. = (−1) .. . . anj an1 . . . ann Now assume that t > 1. Again, we can interchange the tth row with the first row by t − 1 exchanges with the row above, and we get |A| =

11. Determinants

(−1)t−1 |C|, where C 1 ≤ j ≤ n. Therefore

is a matrix satisfying |C1j | = |Atj | for each

|A| = (−1)t−1 |C| = (−1)t−1

n

(−1)j+1 c1j • |C1j | =

j=1

as desired.

211

n

(−1)j+t atj • |Atj |

j=1



1  4  Example: For A =  0 3

7 0 2 1

 0 3   we see that 0  1

3 1 4 5

0 1 3 4 1 = 1 2 4 0 − 7 0 4 1 5 1 3 5 = 16 + 140 − 30 + 0 = 126

3 0 1

4 0 3 + 3 0 2 0 3 1 1

4 − 0 0 3

0 2 1

1 4 5

7 3 0 1 3 |A| = 0 0 1 3 − 2 4 1 1 5 1 3 5 = 0 − 2 + 128 − 0 = 126.

0 3 1

1 7 0 + 4 4 0 3 3 1 1

1 − 0 4 3

7 0 1

3 1 5

|A|

and

Even this method of computing determinants is not easy, however, unless there is a row (or column) of the matrix a significant number of the entries in which are equal to 0. To see the computational overhead of computing the determinant of a general n × n matrix using minors, let us denote the number of arithmetic operations needed to do so by pn . Clearly p1 = 1 and p2 = 3. Suppose that we have already found pn−1 . Then by Proposition 11.11 we see that in order to compute the determinant of an n × n matrix we have to compute the determinants of n matrices of size (n − 1) × (n − 1) and then perform n multiplications and n − 1 additions/subtractions. That is to say, we obtain the recursive formula pn = npn−1 + n + (n − 1) = npn−1 + 2n − 1, when n > 2. Setting tn =

1 n! pn ,

we see that

tn − tn−1 =

1 2 − (n − 1)! n!

212

11. Determinants

and so tn

[tn − tn−1 ] + [tn−1 − tn−2 ] + . . . + [t3 − t2 ] + t2 ! ! 1 2 1 2 − + ... + − +1 = (n − 1)! n! 2! 3! ! ! 1 1 1 1 + ... + − + ... + +1 = 2 (n − 1)! 1! n! 1! 1 1 1 = + ... + + 1 − (n − 1)! 1! n! ! 1 1 1 2 = + + ... + + 1 − n! (n − 1)! 1! n! =

* + 1 1 1 and thus we see that pn = n! n! + (n−1)! + . . . + 1! + 1 −2. But from calculus we know that e, the base of the natural logarithms, has an expansion of the form 1 ec 1 + , e = 1 + + ... + 1! n! (n + 1)! where 0 < c < 1, and so pn = n! e −

! ec − 2. (n + 1)!

If n > 2, we see that 0
t for some 1 ≤ i ≤ t, then the summand sgn(π)aπ(1),1 • aπ(2),2 • . . . • aπ(n),n equals 0. Therefore, we in fact have |A| =

sgn(π)aπ(1),1 • aπ(2),2 • . . . • aπ(n),n ,

π∈U

where U is the subset of Sn consisting of all those permutations π satisfying 1 ≤ π(i) ≤ t for all 1 ≤ i ≤ t and hence, perforce, t + 1 ≤ π(i) ≤ n for all t + 1 ≤ i ≤ n. In other words, each π ∈ U can be considered as the combination of two permutations, one of {1, . . . t}, and the other of {t + 1, . . . n}. Moreover, again as a direct consequence of the definition, sgn(π) is the product of the signa of these two permutations. From this, our result follows immediately. Now assume, inductively, that the result has been established for m and consider a matrix A ∈ Mn×n (K) which can be written in block form     O O A1 O . . . A1 O . . .  O A2 . . .  O  O   . If we set B =  O A2 . . .  as      ... ... O O . . . Am+1 O O . . . Am then, by the case m = 2 and the induction hypothesis, we see that m+1 |Ah | . |A| = |B| • |Am+1 | = h=1

Let A = [aij ] ∈ Mn×n (K) for some associative and commutative unital F -algebra (K, •). We define the adjoint of A to be the matrix adj(A) = [bij ] ∈ Mn×n (K), where bij = (−1)i+j |Aji | for all 1 ≤ i, j ≤ n.

214

11. Determinants



1  −3  Example: If A =  4 1 

0 1 2 1

3 3 1 2

−20  50 adj(A) =   −40 10

 5 1   ∈ M4×4 (R) then 2  5  9 −17 25 −18 −16 −40  . −18 −16 50  9 13 −35

(11.13) Proposition: Let F be a field and let n be a positive integer. If A = [aij ] ∈ Mn×n (F ) then A[adj(A)] = |A|I. In particular, if the matrix A is nonsingular then A−1 = |A|−1 adj(A). Proof: n Suppose that n adj(A) = [bij ]. Then A[adj(A)] = [cij ], where cij = k=1 aik bkj = k=1 (−1)j+k aik |Ajk |. If i = j, then, by Proposition 11.11, this is just |A|. If i = j, this is just |A |, where A is a matrix identical to A in all of its rows except the ith row, and that is equal to the jth row of A. Thus the matrix A has two identical rows, and so by Proposition 11.3, |A | is equal to 0. Hence A[adj(A)] = |A|I, from which we also immediately deduce the second statement since if A is nonsingular then |A| = 0. (11.14) Proposition: Let F be a field, let (K, •) be a associative and commutative unital F -algebra, and let n be a positive integer. If A = [aij ] ∈ Mn×n (K) is an upper-triangular matrix n then |A| = i=1 aii . Proof: We can prove this by induction on n. For the case n = 1, it is immediate. Assume therefore that we have already established it for all matrices in Mn×n (K). Then, by Proposition 11.11, |A| = |AT | = n 1+j aj1 • |Aj1 | = a11 • |A11 |. But, by the induction hypothesis, j=1 (−1) n |A11 | = i=2 aii , and we are done. By Proposition 11.14 we see that in general, from a computational point of view, it is much faster to first perform elementary operations on a matrix to reduce it to upper-triangular form, and then calculate the determinant (making use of the fact, from the definition of a determinant function and from Proposition 11.4, we easily know the determinants of the elementary matrices), than to calculate the determinant directly. When working in associative and commutative unital algebras over a field, or when working with matrices of integers, this presents somewhat of a problem since it is not always possible to divide by nonzero scalars in such contacts. However, various variants on Gaussian elimination which do not involve division have been developed to overcome this.

11. Determinants

215

Combining Propositions 11.4 and 11.14, we see that if A ∈ Mn×n (F ) can be written in the form LU, where L is a lower-triangular matrix and U is an upper-triangular matrix, then |A| is the product of the diagonal elements of L and the diagonal elements of U. (11.15) Proposition (Cramer’s Theorem5 ): Let F be a field and let n be a positive integer.  If A = [aij ] ∈ Mn×n (F ) is a b1  ..  nonsingular matrix and if w =  .  ∈ F n , then the system of bn



 d1   linear equations AX = w has the unique solution v =  ...  in dn which, for each 1 ≤ i ≤ n, we have di = |A|−1 |A(i) |, where A(i) is the matrix formed from A by replacing the ith column of A by w. Proof: If Av = w then |A|v = |A|A−1Av = adj(A)Av = adj(A)w n and so for each 1 ≤ i ≤ n, we have |A|di = j=1 (−1)i+j bj |Aji |. But the expression on the right-hand side of this equation is just, by Proposition 11.11, |A(i) |, developed by minors on the ith column. Cramer’s theorem, published in 1750, was the first systematic method for solving a system of linear equations, though special cases of it were known to Leibnitz 75 years earlier. While it is elegant mathematically, it is clearly not computationally feasible, even when n is only moderately large, as was immediately realized by mathematicians of the time. Indeed, solving a system of linear equations AX = w by Cramer’s method, where A is a nonsingular n × n matrix over a field F, requires 13 n4 − 16 n3 − 13 n2 + 1 1 4 1 3 2 2 2 6 n additions and 3 n + 3 n + 3 n + 3 n − 1 multiplications, which is considerably worse than the methods we have previously studied, for which the number of arithmetic operations necessary grows as n3 , rather than as n4 .

5 Gabriel Cramer was an 18th-century Swiss mathematician and friend of Johann Bernoulli (one of the formulators of calculus) who was among the first to study determinants and their use to solve systems of linear equations.

216

11. Determinants



 2 Example: Consider the system of linear equations AX =  1  , 4   1 −1 1 2 0 . Then |A| = −5 and where A =  1 1 0 −1 2 −1 1 2 1 1 2 0 = −13, |A(2) | = 1 1 0 = 4, and |A(1) | = 1 4 1 4 −1 0 −1 1 −1 2 2 1 = 7. |A(3) | = 1 1 0 4 As a consequence, we see that the unique solution to the equation is  13 1 −4  . 5 −7 We end this chapter with an interesting application of determinants of matrices over the R-algebra R[X]. Let c0 , c 1 , . . . be real numbers and ∞ let us consider the analytic function f : x → i=0 ci xi , which converges for all x in some subset U of R. We know that U = ∅ since surely 0 ∈ U. Given positive integers k and n, we want to find polynomials p(X), q(X) ∈ R[X] of degrees at most k and n respectively, such that all x ∈ U and is the function x → p(x)q(x)−1 − f (x) also converges for ∞ representable there by a power series of the form x → i=1 di xk+n+i . If −1 is called the we find such p and q, then the function x → p(x)q(x) Pad´ e approximant6 to f of type k/n. Padé approximants are very important tools in differential equations and in approximation theory. Example: If f : x → ex =

∞

1 i i=0 i! x

g1 : x →

6

then the function

x2 + 4x + 6 6 − 2x

Henri Pad´ e was a 19th-century French engineer who developed these approximants in the course of his work. Interest in them intensified ´ in the early 20th century when the French mathematician Emile Borel made exensive use of them in his work on analysis.

11. Determinants

217

is a Padé approximant to f of type 2/1 and the function g2 : x →

x2 + 6x + 12 x2 − 6x + 12

is a Padé approximant to f of type 2/2. The following diagram shows a part of the graph of f (broken line) and of g2 (solid line):

If we are given f as above, how do we calculate Padé approximants to it? First of all, define c−i = 0 for all positive integers i. Then, given positive integers k and n, define the matrices Pk/n (X), Qk/n (X) ∈ M(n+1)×(n+1) (R[X]) as follows:   ck−n+2 . . . ck+1 ck−n+1  ck−n+2 ck−n+3 . . . ck+2      . . . Pk/n (X) =    ck+1 . . . ck+n  ck k k−n k−n+1 n+i i ci X n+i−1 . . . i=0 ci X i=0 i=0 ci X and



ck−n+1  ck−n+2  Qk/n (X) =    ck Xn

ck−n+2 ck−n+3 ck+1 X n−1

... ... ... ... ...

 ck+1 ck+2   .  ck+n  1

Then the polynomials p(X) = |Pk/n (X)| and q(X) = |Qk/n (X)| are of the desired size, and our approximant is given by x → p(x)q(x)−1 .

218

11. Determinants

Exercises

Exercise 580 For real numbers a and b, calculate sin(a) sin(b)

cos(a) cos(a) and cos(b) sin(b)

1 i Exercise 581 Calculate −i 1 1−i 0

1+i 0 1

sin(a) . cos(b)

∈ C3 .

Exercise 582 For any real number a, calculate a−6 0 5 a − 4 −1 3 0 − 12 Exercise 583 1 by f : t → 1 t

0 −8 0 12 . a − 2 −6 1 1

Find the image of the function f from R to itself defined 0 −t 1 −1 . 0 −1

Exercise 584 For real numbers a, b, c, and d, show that

a2 b2 c2 d2

(a + 1)2 (b + 1)2 (c + 1)2 (d + 1)2

(a + 2)2 (b + 2)2 (c + 2)2 (d + 2)2

(a + 3)2 (b + 3)2 (c + 3)2 (d + 3)2

= 0.

Exercise 585 Let n be a positive integer and let c be a fixed real number. Let A = [aij ] ∈ Mn×n (R) be the matrix defined by   c if i < j i if i = j . aij =  0 if i > j Calculate |A|.

11. Determinants

219

Exercise 586 If n is a positive integer, we define the nth Hankel7 matrix Hn ∈ Mn×n (R) to be the matrix [aij ] satisfying

0 if i + j − 1 > n . aij = i + j − 1 otherwise Calculate |Hn |.

a Exercise 587 For a, b ∈ R, calculate b a+b

b a+b a+b a a b

.

Exercise 588 Let p(X) = a0 +a1 X +a2 X 2 and q(X) = b0 +b1 X +b2 X 2 be polynomials in C[X]. Show that there exists a complex number c a0 a1 a2 0 0 a0 a1 a2 = 0. satisfying p(c) = q(c) = 0 if and only if b0 b1 b2 0 0 b 0 b1 b2 Exercise 589 Find the set of all pairs (a, b) of real numbers such that a+1 3a b + 3a b + 1 2b b+1 2−b 1 = 0. a+2 0 1 a + 3 b−1 1 a+2 a+b Exercise 590 For a, b, c ∈ R, show that 0 (a − b)2 (a − c)2 2 (b − a) 0 (b − c)2 2 2 (c − a) (c − b) 0

≤ 0.

Exercise 591 Let n be a positive even integer and let c, d ∈ Q. Let A = [aij ] ∈ Mn×n (Q) be the matrix defined by   c if i = j d if i + j = n + 1 . aij =  0 otherwise Calculate |A|.

7

Nineteenth-century German mathematician Hermann Hankel was among the first to recognize and popularize the work of Grassmann.

220

11. Determinants

Exercise 592 Let n be a positive integer and let A = [aij ] ∈ Mn×n (Q) be the tridiagonal matrix defined by

1 if |i − j| ≤ 1 . aij = 0 otherwise Show that

  −1 if n = 3k 1 if n = 3k + 1 |A| =  0 if n = 3k + 2

for some nonnegative integer k. Exercise 593 Find integers a, b, and c for which a+b c c a b+c a b b a+c is divisible by 8. Exercise 594 Let n be a positive integer and let A ∈ Mn×n (Q) be a nonsingular matrix satisfying the condition that all of the entries of A and of A−1 are integers. Show that |A| = ±1. Exercise 595 For elements a, b, and −2a a + b a + b −2b a+c b+c

c of a field F, calculate a + c b + c . −2c

Exercise 596 We know that the integers 23028, 2 3 and 61902 are all divisible by 19. Show that 8 0 6 divisible by 19.

31882, 86469, 6327, 3 0 2 8 1 8 8 2 6 4 6 9 is also 6 3 2 7 1 9 0 2

Exercise 597 Let q ∈ Q. matrices in  Show that there are infinitely-many  2 2 3 M3×3 (Q) of the form  3q + 2 4q + 2 5q + 3  , where a < b < c, a b c the determinant of which equals q. Exercise 598 Let n be a positive integer and let F be a field. Let A ∈ Mn×n (F ) be a nonsingular matrix which can be written in block form ! A11 A12 , where A11 ∈ Mk×k (F ) for some integer k < n. A= A21 A22

11. Determinants

Write A−1

as

|A11 | = |A| · |B22 |.

B11 B21

B12 B22

221

! , where B11 ∈ Mk×k (F ). Show that

a 1 1 1 1 a 2 3 Exercise 599 Find all real numbers a for which = 0. 0 −1 0 1 −1 1 1 2 Exercise 600 Let a1 , a2 , . . . be a sequence of real numbers. For each positive integer n, define the nth continuant cn of the sequence to be the determinant of the tridiagonal matrix An = [aij ] ∈ Mn×x (R) given by  ai if i = j    −1 if i = j − 1 aij = . 1 if i = j + 1    0 otherwise Show that cn = an cn−1 + cn−2 for all n > 2. Exercise 601 Let n > 1 be an integer, let d be a real number, and let A = [aij ] ∈ Mn×n (R) be the matrix defined as follows:   0 if i = j 1 if i > 1 and j = 1 or i = 1 and j > 1 . aij =  d otherwise Show that |A| = (−1)n−1 (n − 1)dn−2 . Exercise 602 Let b1 , . . . , bn be nonzero real numbers and let A = [aij ] ∈ Mn×n (R) be the matrix defined as follows:

aij =

1 + bj 1

if i = j . otherwise

Calculate |A|. Exercise 603 Let A = [aij ] ∈ M4×4 (Q) be a matrix each entry of which is either −2 or 3. Show that |A| is an integer multiple of 125. Exercise 604 Let a, b, c, and d be real numbers not all of which are   a b c d  b −a d −c   ∈ M4×4 (R) is equal to 0. Show that the matrix   c −d −a b  d c −b −a nonsingular.

222

11. Determinants

Exercise 605 Does there exist a rational number a satisfying the condi  1 a 0 1  ∈ M3×3 (Q) is nonsingular? tion that the matrix  a 1 −1 a −1 Exercise 606 Find all matrices I = A ∈ M2×2 (R) satisfying A3 = I. Exercise 607 1 a dition 1 b 1 c

Find all triples (a, b, c) of real numbers satisfying the con a3 b3 = (b − c)(c − a)(a − b)(a + b + c). c3

Exercise 608 Let n be a positive integer, let A = [aij ] ∈ Mn×n (C) and let B = [bij ] ∈ Mn×n (C) be defined by bij = aji for each 1 ≤ i, j ≤ n. Show that |AB| is a nonnegative real number. 1 logb a Exercise 609 Calculate for given positive real numbers 1 loga b a and b. 1 a3 a a2 3 a a2 a 1 Exercise 610 Let F be a field. Calculate 2 3 for 1 3 2a2 3a 4a 4a 3a 2a 1 any a ∈ F. cos(a) sin(a) cos(a) sin(a) cos(2a) sin(2a) 2 cos(2a) 2 sin(2a) for Exercise 611 Calculate cos(3a) sin(3a) 3 cos(3a) 3 sin(3a) cos(4a) sin(4a) 4 cos(4a) 4 sin(4a) a ∈ R. Exercise 612 Let n be a positive integer and let A = [aij ] ∈ Mn×n (R) be the matrix defined by

0 if i = j aij = . 1 otherwise Calculate |A|.



 3 −1 1 2 4  ∈ M3×3 (R). Calculate adj(A). Exercise 613 Let A =  0 1 −1 1   1 1 0 Exercise 614 Let F = GF (2) and let A =  0 1 1  ∈ M3×3 (F ). 1 1 1 Calculate adj(A).

11. Determinants

223

Exercise 615 Let F be a field, let n be a positive integer, and let A, B ∈ Mn×n (F ). Is it necessarily true that adj(AB) = adj(A) adj(B)? Exercise 616 Let F be a field, let n be a positive integer, and let A ∈ Mn×n (F ). Is it necessarily true that adj(AT ) = adj(A)T ? Exercise 617 Let F be a field, let n be a positive integer, and let the matrices A, B ∈ Mn×n (F ) be nonsingular. Show that adj(B −1 AB) = B −1 adj(A)B. Exercise 618 Let F be a field, let n be a positive integer, and let A, B ∈ Mn×n (F ) be matrices satisfying B = O and AB = O. Show that |A| = 0.   1 2 3 Exercise 619 Let A =  1 3 4  ∈ M3×3 (R). Use the adjoint of A 1 4 3 to calculate A−1 . Exercise 620 Let F be a field, let n be a positive integer, and let A = [aij ] ∈ Mn×n (F ). Let B = [bij ] ∈ Mn×n (F ) defined by bij = (−1)i+j aij for all 1 ≤ i, j ≤ n. Show that |A| = |B|. Exercise 621 Let F be a field, let n be a positive integer, and let A = [aij ] ∈ Mn×n (F ). Let B = [bij ] ∈ Mn×n (F ) defined by bij = (−1)i+j+1 aij for all 1 ≤ i, j ≤ n. Show that (−1)n |A| = |B|. Exercise 622 Let n be a positive integer and let π ∈ Sn . Let A ∈ Mn×n (Q) be the permutation matrix defined by π. Calculate |A|. Exercise 623 Is the set of all permutation matrices in Mn×n (Q) closed under multiplication? Is the inverse of a permutation matrix a permutation matrix? Exercise 624 Let A = [aij ] ∈ M3×3 (R) be a matrix in which ai2 = 0 for all 1 ≤ i ≤ 3. Denote the minor of aij for all 1 ≤ i, j ≤ n by Aij . Show that 1 A11 A13 1 A11 A13 1 A21 A23 + + . |A| = a12 A31 A32 a22 A31 A33 a32 A21 A22 Exercise 625 Let F be a field, let n be a positive integer, and let A = [aij ] ∈ Mn×n (F ) be nonsingular. Show that adj(adj(A)) = |A|n−2 A. Exercise 626 Let a and b be real numbers and let n be an integer greater than 2. Let D = [dij ] ∈ Mn×n (R) be the matrix defined by dij = sin(ia + jb) for all 1 ≤ i, j ≤ n. Show that |D| = 0.

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11. Determinants

Exercise 627

Let F be a field a b b a c d e + e f g g f

and let a, b, c, d, e, f, g ∈ F. Show that b b a b b c d + d e c = 0. g g f g g

Exercise 628 Let F be a field, let n be a positive integer, and let A = [aij ] ∈ Mn×n (F ). Let B = [bij ] ∈ Mn×n (F ) be the matrix defined by

aij + ai,j+1 if j < n bij = . otherwise ain Show that |B| = |A|. Exercise 629 Let k and n be integers greater than 1. Let F be a field and let A = [aij ] be a matrix in Mk×n (F ), the upper row of which contains at least one nonzero entry. For each 2 ≤ i ≤ k and each a11 a1j . Show that the rank of the matrix 2 ≤ j ≤ n, let dij = ai1 aij 

d22  D =  ... dk2

... ...

 d2n ..  ∈ M (k−1)×(n−1) (F ) .  dkn

is r − 1, where r is the rank of A. Exercise 630 Let F be a field, let a = b be elements of F, and let A, B ∈ M2×2 (F ) be matrices satisfying the condition that |A + hB| ∈ {a, b} for h = 1, 2, 3, 4, 5. Show that |A + 9B| ∈ {a, b}. Exercise 631 Let F be a field and let a, b, c ∈ F. Make use of the   b c 0 matrix  a 0 c  in order to calculate the determinant of the matrix 0 a b   2 ab ac b + c2 .  bc ab a2 + c2 2 2 ac bc a +b Exercise 632 Let A ∈ Mn×n (C) be a nonsingular matrix, which we will write in the form B + iC, where B, C ∈ Mn×n (R). Show that there is a real number d such that the matrix B + dC ∈ Mn×n (R) is nonsingular. Exercise 633 Let F be a field and let n be a positive integer. Let A ∈ Mn×n (F ) be a matrix having the property that the sum of all evennumbered columns (considered as vectors in F n ) of A equals the sum of all odd-numbered columns of A. What is |A|?

11. Determinants

225

Exercise 634 Let V = R2 and let f : V 3 → R be the function defined as   a1 b1 1 ! v1 ai for i = 1, 2, 3, then f :  v2  → a2 b2 1 . follows: if vi = bi a3 b3 1 v3 Show that f (v1 , v2 , v3 ) = f (v4 , v2 , v3 ) + f (v1 , v4 , v3 ) + f (v1 , v2 , v4 ) for all v1 , v2 , v3 , v4 ∈ V. Exercise 635 Let F be a field and let n be a positive integer. Let D = [dij ] ∈ Mn×n (F ) be the matrix defined by dij = 1 for all 1 ≤ i, j ≤ n. Show that for any matrix A ∈ Mn×n (F ) precisely one of the following conditions holds: (1) There is a unique scalar a ∈ F such that A + aD is singular; (2) A + aD is singular for all scalars a ∈ F ; (3) A + aD is nonsingular for all scalars a ∈ F. Exercise 636 Let A, B, C, D ∈ M2×2 (R) and let M be the matrix ! A B ∈ M4×4 (R). If all of the “formal determinants” AD − BC, C D AD − CB, DA − BC, and DA − CB are nonsingular, is M necessarily nonsingular? Exercise 637 Let A, B, C, D ∈ M2×2 (R) and let M be the matrix ! A B ∈ M4×4 (R). If M is a nonsingular matrix matrix, is at least C D one of the “formal determinants” AD − BC, AD − CB, DA − BC, and DA − CB also nonsingular? Exercise 638 Let n > 1 be an integer and let A = [aij ] ∈ Mn×n (Q) be a matrix satisfying the condition that each aij is either equal to 1 or to −1. Show that |A| is an integer multiple of 2n−1 . Exercise 639 If a, b, c, d, e, f are nonzero elements of a field F, show 0 a2 b2 c2 0 ad be cf 2 a 0 f 2 e2 ad 0 cf be that 2 2 2 = . b2 f 2 02 d be cf 0 ad c e d 0 cf be ad 0 Exercise 640 Let n be a positive integer and let c1 , . . . , cn be distinct real numbers transcendental over Q. For 1 ≤ h ≤ n, let ph (X) = h−1 i i=0 ai X ∈ Q[X] be a polynomial of degree h − 1. Let A = [pi (cj )] ∈ (cj − ci ). Mn×n (R). Show that |A| = (a0 · . . . · an−1 ) i<j

Exercise 641 Let n be a positive integer and let c1 , . . . , cn be distinct real numbers transcendental over Q. For each 1 ≤ i, j ≤ n, set dij =

226

11. Determinants

cji − c−j and let A = [dij ] ∈ Mn×n (R). Show that i |A| = (c1 · . . . · cn )−n

i<j

Exercise 642 Let

[(ci − cj )(1 − ci cj )]

n

(c2i − 1).

i=1

a, b, c, d be elements of a field F. Solve the equation 0 1 −1 1 a b c d 1 c b c d a d a = X . 1 d c d a b a b 1 a d a b c b c

Exercise 643 Let a, b, and c be nonzero real numbers. Under which 0 a−X b − x 0 c − X = 0 have more conditions does the equation −a − X −b − X −c − X 0 than one solution? Exercise 644 Use determinants to show that there is no matrix A ∈  1 0 0 0  0 2 0 0   M4×4 (Q) satisfying the condition that A4 =   0 0 1 0 . 0 0 0 1 Exercise 645 Let A = [aij ] ∈ Mn×n (R) be a matrix satisfying the condition |aii | > j=i |aij | for all 1 ≤ i ≤ n. Show that |A| = 0. Exercise 646 Let F be a field and let a, b, c ∈ F. Is a b c 0 −a b c 0 b a 0 c b −a 0 c c 0 a b = c 0 −a b 0 c b a 0 c b −a

it true that ?

Exercise 647 Let F be a field and let n > 2 be an integer. Give an example of a matrix A ∈ Mn×n (F ) all of the entries in which are nonzero, satisfying adj(A) = O. Exercise 648 Let F be a field and let n > 2 be an integer. | adj(A)| = |A|n−1 for all A ∈ Mn×n (F ).

Show that

Exercise 649 Is the function adj : M2×2 (R) → M2×2 (R) epic?   s 0 t Exercise 650 For real numbers s and t, let A(s, t) =  1 1 1  t 0 1 and let B(s, t) = adj(A(s, t)). Find the set of all real numbers s satisfying the condition that |A(s, t)| = |B(s, t)| for all t ∈ R.

11. Determinants

227

Exercise 651 Let F be a field. Does there exist a matrix A in M3×3 (F ) satisfying the condition that the rank of adj(A) equals 2? Exercise 652 Let n be a positive integer and for all 1 ≤ j ≤ n, let mj be a positive Define the matrix A = [aij ] ∈ Mn×n (Q) by setting +i−1integer. for all 1 ≤ i, j ≤ n. Calculate |A|. aij = mjj−1 Exercise 653 Let a and b be distinct elements of a field F and let n be a positive integer. Let A(n) = [aij ] ∈ Mn×n (F ) be the matrix defined by

a if i = j . aij = b otherwise Use induction on n to prove that |A(n)| = [a + (n − 1)b](a − b)n−1 . Exercise 654 Let n be a positive integer and pick integers 1 ≤ h, k ≤ n. Let f, g ∈ RR be the functions defined by

|Eh,c | if c = 0 f : c → 0 if c = 0 and g : c → |Ehk;c |. Are these functions continuous? Exercise 655 Let n be a positive integer and let A ∈ Mn×n (Q) be a nonsingular matrix the entries of which are integers and the determinant of which is ±1. Show that all of the entries of A−1 are integers. Exercise 656 Let F be a field and let A ∈ M2×2 (F ). Show that the matrix A2 + |A|I belongs to the subspace of M2×2 (F ) generated by {A}. Exercise 657 Let A = [aij ] ∈ M3×3 (Q) be a matrix all of the entries of which are nonnegative one-digit integers. Let d be a positive integer dividing the three-digit integers a11 a12 a13 , a21 a22 a23 , and a31 a32 a33 . Show that d divides |A|. Exercise 658 Let n be a positive integer and let F be a field. Let A ∈ Mn×n (F ) be a matrix satisfying the condition that |A + B| = |A| for all B ∈ Mn×n (F ). Show that A = O. Exercise 659 Let n be an odd positive integer let A ∈ Mn×n (R). Show that there exists a diagonal matrix B the diagonal entries of which are ±1 such that A + B is nonsingular. Exercise 660 Let n > 1 be an integer and let F be a field. Show that there exist subspaces W and Y of Mn×n (F ) satisfying Mn×n (F ) = W ⊕ Y such that the restrictions of the determinant function δ n to W and to Y are linear transformations.

228

11. Determinants

Exercise 661 Let n > 1 be an integer and let B be the set of all of the nonsingular matrices in Mn×n (R) all of the entries of which are either 1 or 0. Show that in every matrix in B there are at least n − 1 entries which are equal to 0 and that there exists a matrix in B in which there are precisely n − 1 entries equal to 0. Exercise 662 Let A be a matrix formed by permuting the rows or columns of a Hadamard matrix. Is A necessarily a Hadamard matrix? Exercise 663 Let V be a vector space of finite dimension n over a field F and let {v1 , . . . , vn } be a given basis for V. Let U be the subset of n V consisting of all vectors of the form ya = i=1 ai−1 vi , for 0 = a ∈ F. Show that any subset of U having n elements is a basis for V. Exercise 664 Let F be a field and let n be an even positive integer. Let A ∈ Mn×n (F ) be a matrix which can be written in block form as [Aij ] , ! ! 0 ci 0 0 where Aij = if i = j, and Aij = otherwise. −ci 0 0 0 Calculate the Pfaffian of A. √ Exercise 665 Let c = 12 1 + i 3 . Find the set of all real numbers a a 1 1 such that 1 c c2 ∈ R. 1 c2 c Exercise 666 Let a, b, c, d be elements of a field F. Calculate a b c d b a d c c d a b . d c b a

12 Eigenvalues and eigenvectors

One of the central problems in linear algebra is this: given a vector space V finitely generated over a field F, and given an endomorphism α of V, is there a way to select a basis B of V so that the matrix ΦBB (α) is as nice as possible? In this chapter we will begin by defining some basic notions which will help us address this problem. Let V be a vector space over a field F and let α ∈ End(V ). A scalar c ∈ F is an eigenvalue of α if and only if there exists a vector v = 0V satisfying α(v) = cv. Such a vector is called an eigenvector1 of α associated with the eigenvalue c. Thus we see that a nonzero vector v ∈ V is an eigenvector of α if and only if the subspace F v of V is invariant under α. Every eigenvector of α is associated with a unique eigenvalue of α but any eigenvalue has, as a rule, many eigenvectors associated with it. The set of all eigenvalues of α is called the spectrum of α and is denoted by spec(α). Thus, c ∈ spec(α) if and only if the endomorphism cσ 1 − α of V is not monic. 1 The terms “eigenvalue” and “eigenvector” are due to Hilbert. Eigenvalues and eigenvectors are sometimes called characteristic values and characteristic vectors respectively, based on terminology used by Cauchy. Sylvester coined the term “latent values” since, as he put it, such scalars are “latent in a somewhat similar sense as vapour may be said to be latent in water or smoke in a tobacco-leaf”.

229

230

12. Eigenvalues and eigenvectors

Example: The spectrum of α ∈ End(V ) may be empty. For example, ! ! a −b → then spec(α) = ∅. if α ∈ End R2 is defined by α : b a More generally, if V is any vector space over R and if α ∈ End(V ) satisfies α2 = −σ 1 , then spec(α) = ∅. To see this, note that if v is an eigenvector corresponding to an eigenvalue c then −v = α2 (v) = c2 v and so (c2 + 1)v = 0V , implying that c2 = −1, which is impossible for a real number c. ! ! 2 a b be defined by α : → . Example: Let α ∈ End R b a ! a Then c ∈ spec(α) if and only if there exists a vector satisfying b ! ! ! b ca a = . Therefore we see that spec(α) = {−1, 1}, where a cb −a ! a is an example of an eigenvector of α associated with −1 and is a an example of an eigenvector of α associated with 1, for any 0 = a ∈ R. Example: Let V be the vector space of all infinitely-differentiable functions from R to itself and let δ be the endomorphism of V which assigns to each such function its derivative. Then a function f, which is not the 0-function, is an eigenvector of δ if and only if there exists a scalar c ∈ R such that δ(f ) = cf. For any real number c, there is indeed such a function in V , namely the function x → ecx . Thus spec(δ) = R. The set of all eigenvectors of δ associated with c is {aecx | a = 0}. This fact has important applications in the theory of differential equations2 . Let α be an endomorphism of a vector space V of a field F having an eigenvalue c. If β ∈ Aut(V ) then c is also an eigenvalue of βαβ −1 . Indeed, if v is an eigenvector of α associated with c then

2

The first use of eigenvalues to study differential equations is due to the French mathematician Jean d’Alembert, one of the foremost researchers of the 18th century. Important solutions of eigenvalue problems for second-order differential equations were obtained in the 19th century by Swiss mathematician Charles-Fran¸ cois Sturm and French mathematician Joseph Liouville.


231

βαβ −1 (β(v)) = βα(v) = β(cv) = cβ(v) and β(v) = 0V since β is an automorphism. Therefore β(v) is an eigenvector of βαβ −1 associated with c. n Similarly, let p(X) = i=0 bi X i ∈ F [X]. If v ∈ V is an eigenvector of α associated with an eigenvalue c, then v is also an eigenvector of with the eigenvalue p(c), since p(α)v = )n associated n p(α) i∈ End(V i b α (v) = b c v = p(c)v. In particular, we see that, for any i i i=0 i=0 positive integer n, the vector v is an eigenvector of αn associated with the eigenvalue cn . Let V be a vector space over a field F and let α be an endomorphism of V. A vector v ∈ V is a fixed point of α if and only if α(v) = v. It is clear that 0V is a fixed point of every endomorphism of V and a nonzero vector v is a fixed point of α if and only if 1 ∈ spec(α) and v is an eigenvalue of α associated with 1. (12.1) Proposition: Let V be a vector space over a field F and let α be an endomorphism of V having an eigenvalue c. The subset W composed of 0V and all eigenvectors of α associated to c is a subspace of V. Proof: If w, w ∈ W and a ∈ F then α(w + w ) = α(w) + α(w ) = cw + cw = c(w + w ) and α(aw) = aα(w) = a(cw) = c(aw) and so both w + w and aw belong to W, proving that W is a subspace of V. Let V be a vector space over a field F and let α be an endomorphism of V having an eigenvalue c. The subset W composed of 0V and all eigenvalues of α associated with c, which we know by Proposition 12.1 is a subspace of V, is called the eigenspace of α associated with c. In particular, if 1 is an eigenvalue of α then the fixed space of α is the eigenspace associated with 1. If 1 ∈ / spec(α) then the fixed space of α is taken to be {0V }. Example:

Let α be the endomorphism of R3 defined by     a a α :  b  →  0  . c c

Then 1 ∈ spec(α) and the eigenspace of α associated with 1 (namely      0   1 the fixed space of α) is R  0  ,  0  .   0 1

232


Example: Let V =4 C(0, 1) and let α be the endomorphism of V x defined by α(f ) : x → 0 cos(π[x − t])f (t)dt for all f ∈ V. To find the eigenvalues of α, recall the trigonometric identity cos(π[x − t]) = cos(πx) cos(πt) + sin(πx) sin(πt). Using this identity, we see that if f ∈ V then ! 6 6 x cos(πt)f (t)dt cos(πx) + α(f ) : x → 0

!

x

sin(πt)f (t)dt sin(πx)

0

and so the image of α is contained in the subspace W = R{g1 , g2 } of V, where g1 : x → cos(πx) and g2 : x → sin(πx). It is easy to see that α(g1 ) = 12 g1 and α(g2 ) = 12 g2 , so both of these functions are {g1 , g2 } is eigenvectors of α associated with the eigenvalue 12.. Moreover, / linearly independent. Thus we see that spec(α) = 12 and the eigenspace associated with this sole eigenvalue is W. (12.2) Proposition: Let V be a vector space finitely generated over a field F and let α be an endomorphism of V . Then the following conditions on a scalar c are equivalent: (1) c is an eigenvalue of α; / Aut(V ); (2) cσ 1 − α ∈ (3) If A = ΦBB (α) for some basis B of V, then |cI − A| = 0.

Proof: (1) ⇔ (2): Condition (1) is satisfied if and only if there exists a nonzero vector v ∈ V satisfying α(v) = cv, i.e. if and only if (cσ 1 − α) (v) = 0V . This is true if and only if ker(cσ 1 − α) = {0V }. Since V is finitely generated, by Proposition 7.3 we know that this is true if and only if condition (2) holds. (2) ⇔ (3): This is a direct consequence of the fact that a matrix is nonsingular if and only if its determinant is nonzero. From Proposition 12.2, we see how to define eigenvalues of square matrices over a field: if F is a field and n is a positive integer, then c ∈ F is an eigenvalue of a matrix A ∈ Mn×n (F ) if and only if |cI −A| = 0, namely if and only if the matrix cI − A is singular. The set of all eigenvalues of A will be denoted by spec(A). In particular, we observe that a matrix   0   A is nonsingular if and only if 0 ∈ / spec(A). A vector  ...  = v ∈ F n 0 is an eigenvector of A associated with the eigenvalue c if and only if


233



Av = cv. The subset of F n

 0   consisting of  ...  and all eigenvectors 0

of A associated with c is a subspace of F n called the eigenspace associated with c. In the case that F equals R or C, the number ρ(A) = max{|c| | c ∈ spec(A)} is called the spectral radius of the matrix A, and plays a very important part in the numerical analysis of matrices. Note that if F = C, then ρ(A) is just the radius of the smallest circle in the complex plane, centered at the origin, containing spec(A). Moreover, −1 spec(A) consists precisely of the poles of the function z → |zI − A| . This observation allows the use of powerful techniques of complex analysis in the study of the spectra of complex matrices. Example: It is not necessarily true that ρ(AB) =! ρ(A)ρ(B) for square ! 0 2 0 0 matrices A and B. For example, if A = and B = 0 0 2 0 in M2×2 (R), then ρ(A) = 0 = ρ(B), whereas ρ(AB) = 4. T GivenT a matrix A ∈ Mn×n (F ), weT note that |cI − A| = |(cI − A) | = cI − A and so spec(A) = spec(A ). However, for each such common eigenvalue, the associated eigenvectors may be different.

Example: Let F be a field and let n be a positive integer. If     a1 b1     v =  ...  and w =  ...  are vectors in F n , then we have already an

bn

noted that their exterior product v ∧ w = vwT ∈ Mn×n (F ) and their interior product v w, satisfies v T w = [v w] ∈ M1×1 (F ). Direct calculation shows that (v ∧ w)v = (v w)v and so v w is an eigenvalue of v ∧ w associated with the eigenvector v. 

1 Example: Let A =  −1 0

 1 −2 2 1  ∈ M3×3 (R). Then spec(A) = 1 −1

{−1, 1, 2} and so this is also spec(AT ).



 1 (1) The eigenspace of A associated with −1 is R  0  and the 1   1 eigenspace of AT associated with −1 is R  2  ; −7

234




 3 (2) The eigenspace of A associated with 1 is R  2  and the 1   −1 eigenspace of AT associated with 1 is R  0  ; 1   1 (3) The eigenspace of A associated with 2 is R  3  and the 1   −1 eigenspace of AT associated with 2 is R  1  . 1 Example: Let n be a positive integer and let A = [auj ] be an n × n Markov matrix, which we will consider as an element of Mn×n (C). We   b1   claim that ρ(A) ≤ 1. Indeed, let c ∈ spec(A) and let v =  ...  ∈ Cn bn be an eigenvector associated with c. Let 1 ≤ h ≤ n satisfy the condition that |bi | ≤ |bh | for all 1 ≤ i ≤ n. Then Av = cv implies, in particular, n that j=1 ahj bj = cbh and so   n n n ahj bj ≤ ahj |bj | ≤  ahj  |bh | = |bh | . |c| · |bh | = |cbh | = j=1 j=1 j=1 Hence |c| ≤ 1, as claimed. Example: Let n be a positive integer and let A ∈ Mn×n (R) be a skew-symmetric matrix. We claim that spec(A) ⊆ {0}, with equality when n is odd. Indeed, let c ∈ spec(A) and let v ∈ Rn be an eigenvector of A associated with c. Then −AT v = Av = cv and so −AT (Av) = −AT (cv) = c(−AT v) = c2 v. Therefore −(Av Av) =   b1   −v T AT Av = c2 v T v = c2 (v v). But if y =  ...  is any vector in Rn , bn



 0 n   then yy = i=1 b2i ≥ 0, with equality if and only if y =  ...  . Since v 0 is nonzero, we conclude that we must have c2 = 0 and so c = 0. Therefore spec(A) ⊆ {0}. If n is odd then, by the remark after Proposition 11.7, we know that A is singular and so 0 ∈ spec(A), establishing equality.


235

Example: Let n be a positive integer and let A ∈ Mn×n (C). If c is a nonzero eigenvalue of A and if v ∈ Cn is an eigenvector associated with c then, by Proposition 11.13, we know that |A| v = adj(A)Av = c [adj(A)] v and so [adj(A)] v = c−1 |A| v. Thus v is also an eigenvector of adj(A) associated with the eigenvalue c−1 |A| . If F is a field, if n is a positive integer, and if A ∈ Mn×n (F ) is a matrix having eigenvalue c, then |cI −A| = 0 and so by Proposition 11.13 we see that (cI−A) adj(cI−A) = O, and so A[adj(cI−A)] = c[adj(cI−A)]. From this we conclude that each of the columns of adj(cI −A) must belong to the eigenspace of A associated with c.   0 1 0 0 1  ∈ M3×3 (R). Then one can Example: Let A =  0 4 −17 8 √ √ calculate that spec(A) = {2 − 3, 2 + 3, 4}. Moreover, adj(4I − A) =   1 −4 1  4 −16 4  and it is easy to check that the columns of this matrix 16 −64 16 are indeed eigenvectors of A associated with 4. (12.3) Proposition: If V is a vector space finitely generated over a field F and if α, β ∈ End(V ) then spec(αβ) = spec(βα). Proof: Let c ∈ spec(αβ). If c = 0, this means that αβ ∈ / Aut(V ). Therefore either α or β is not an automorphism of V, and so βα ∈ / Aut(V ) as well. Therefore we can assume c = 0. Let v be an eigenvector of αβ associated with c and let w = β(v). Then α(w) = αβ(v) = cv = 0V and so w = 0V . Moreover, βα(w) = βαβ(v) = β(cv) = cβ(v) = cw and so w is an eigenvector of βα associated with c. Thus spec(αβ) ⊆ spec(βα). A similar argument shows the reverse inclusion, and so we have equality. In particular, as a consequence of Proposition 12.3, we see that if F is a field, if n is a positive integer, and if A, B ∈ Mn×n (F ) then spec(AB) = spec(BA). As we noted at the beginning of the chapter, if we are given a vector space V finitely generated over a field F and an endomorphism α of V, we would like to find, to the extent possible, a basis B of V such that the matrix ΦBB (α) is nice, in the sense that it is amenable to quick and accurate calculations. Let V be a vector space over a field F (not necessarily finitely generated) and let α ∈ End(V ). Then α is

236


diagonalizable if and only if there exists a basis B of V composed of eigenvectors of α. Example: We have already seen that the set B of all functions in RR of the form x → eax , for some a ∈ R, is linearly independent. Therefore W = RB is a subspace of RR which is not finitely generated, and B is a basis for W. Let α be the endomorphism of W which assigns to each f ∈ W its derivative. Since each element of B is an eigenvector of α, we see that α is diagonalizable. The following result characterizes the diagonalizable endomorphisms of finitely-generated vector spaces. (12.4) Proposition: Let V be a vector space finitely generated over a field F and let α ∈ End(V ). Then the following conditions on a basis B = {v1 , . . . , vn } are equivalent: (1) vi is an eigenvector of α for each 1 ≤ i ≤ n; (2) ΦBB (α) is a diagonal matrix. Proof: (1) ⇒ (2): By (1) we know that for each 1 ≤ i ≤ n there exists a scalar ci satisfying α(vi ) = ci vi and so, by definition, ΦBB (α) is the diagonal matrix [aij ] given by

ci if i = j . aij = 0 otherwise (2) ⇒ (1): If ΦBB (α) = [aij ] is a diagonal matrix then for each 1 ≤ i ≤ n we have α(vi ) = aii vi and so vi is an eigenvector of α for each 1 ≤ i ≤ n. Let V be a vector space over a field F and let α ∈ End(V ). If B is a basis of V made up of eigenvectors of α then, as we have seen above, the elements of B are also eigenvectors of p(α) for any polynomial p(X) ∈ F [X]. We need not stick to polynomials: suppose that each v ∈ B is an eigenvector of α associated with an eigenvalue cv of α. Given any function whatsoever f : spec(α) → the endomorphism F, we can define a v → a f (α) of V by setting f (α) : v∈B v v∈B v f (cv )v and the elements of B are also eigenvectors of f (α). We note that if f and g are functions from spec(α) to F then f (α)g(α) = g(α)f (α). Now assume that V is finitely generated over F and that B = {v1 , . . . , vn } is a basis of V made up of eigenvectors of α ∈ End(V ). For each 1 ≤ i ≤ n, let ci be the eigenvalue of α associated with vi . We have already seen that for each such i there exists a polynomial pi (X), namely the Lagrange interpolation polynomial, satisfying the condition that

1 if i = j . pi (cj ) = 0 otherwise


237

Thus, given a function f : spec(α) → F, the polynomial p(X) = n i=1 f (ci )pi (X) satisfies p(ci ) = f (ci ) for all 1 ≤ i ≤ n, and so p(α) = f (α). Thus, for finitely-generated vector spaces, the above generalization does not in fact contribute anything new; it is important however, in the case of vector spaces which are not finitely generated. We now show that the size of the spectrum of an endomorphism of a finitely-generated vector space is limited. (12.5) Proposition: Let V be a vector space over a field F and let α ∈ End(V ). If c1 , . . . , ck are distinct eigenvalues of α and if vi is an eigenvector of α associated with ci for each 1 ≤ i ≤ k, then the set {v1 , . . . , vk } is linearly independent. Proof: Assume that the set {v1 , . . . , vk } is linearly dependent. Since v1 = 0V , we know that the set {v1 } is linearly independent. Thus there exists an integer 1 ≤ t < k such that the set {v1 , . . . , vt } is linearly independent but {v1 , . . . , vt+1 } is linearly dependent. In other words, there exist scalars a1 , . . . , at+1 , not all ofwhich are equal to 0, such t+1 t+1 t+1 that = i=1 ai ct+1 vi . i=1 ai vi = 0V and so 0V = ct+1 i=1 ai vi t+1 t+1 t+1 On the other hand, 0V = α i=1 ai vi = i=1 ai α(vi ) = i=1 ai ci vi . t+1 t+1 t Therefore 0V = i=1 ai ci vi − i=1 ai ct+1 vi = i=1 ai (ci − ct+1 )vi . But the set {v1 , . . . , vt } is linearly independent and so ai (ci − ct+1 ) = 0 for all 1 ≤ i ≤ t. Since, by assumption, ci = ct+1 for all 1 ≤ i ≤ t, this implies that ai = 0 for all 1 ≤ i ≤ t and hence at+1 = 0 as well, which is a contradiction. Thus the set {v1 , . . . , vk } must be linearly independent. Thus we see that if F is a field and if A ∈ Mn×n (F ), then spec(A) can have at most n elements. In particular, if F has more than n elements,   0  ..  then there exists an element c ∈ F spec(A), and so (cI − A)v =  .  

 0   for all v =  ...  . This implies that cI − A is nonsingular. 0

0

From Proposition 12.5 we see that if α is a an endomorphism of a vector space V over a field F having distinct eigenvalues c1 , . . . , ck , and if Wi is the eigenspace associated with ci for all 1 ≤ i ≤ t, then the collection {W1 , . . . , Wk } of subspaces of V is independent. Moreover, If

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V is finitely generated over F then the number of elements in spec(α) is no greater than dim(V ). (12.6) Proposition: Let V be a vector space of finite dimension n over a field F. Then any endomorphism α of V having n distinct eigenvalues is diagonalizable. Proof: This is a direct consequence of Proposition 12.4 and Proposition 12.5. ! ! a 3a − b 2 → . Example: Let α ∈ End(R ) be defined by α : b 3b − a ! ! ! 1 2 1 Then α = and so is an eigenvector of α associated 1 2 1 ! ! ! 1 4 1 with the eigenvalue 2. Also, α = and so −1 −4 −1 is an eigenvector of α associated with the eigenvalue 4. Thus B = !

! !2 0 1 1 . , is a basis for R2 and ΦBB (α) = 0 4 1 −1 a b

!

a+b b

!

Example: Let α ∈ End(R ) be defined by α : → . If ! ! ! ! a 0 a a = and α =c then cb = b and a + b = ca, b 0 b b and this can happen only when b = 0 and c = 1. Thus spec(α) = {1} ! 0 and the eigenspace associated with this sole eigenvalue is R . Since 1 2

this is not all of R2 , we know that there is no basis of R2 made up of eigenvectors of α and hence α is not diagonalizable. Note that the converse of Proposition 12.6 is false, as we easily see by taking α = σ 1 . From the above, we know that if A ∈ Mn×n (R) then the matrix has at most n distinct eigenvalues. However, it may have many less than that. If we assume that the entries of this matrix were chosen independently and randomly from a standard normal distribution, how many distinct eigenvalues should we expect? American mathematicians Alan Edelman, Eric Kostlan and Michael Shub have shown that if εn denotes the mathematical expectancy7for the number of eigenvalues of such a matrix in R, then lim

n→∞

√1 εn n

=

2 π.

The situation over the complex numbers is quite dif-

ferent. Given a matrix A ∈ Mn×n (C) one can, with probability 1, pick


239

a matrix B ∈ Mn×n (C) as near to A as we wish, which has n distinct eigenvalues in C. If F is a field, if n is a positive integer, and if A ∈ Mn×n (F ), then we can consider the matrix of polynomials XI − A ∈ Mn×n (F [X]). The determinant of this matrix, |XI − A|, is a polynomial in F [X] called the characteristic polynomial of A. Note that this polynomial is always monic and of degree n. 

1 Example: The characteristic polynomial of  2 4 is X 3 − 3X 2 − 5X + 27.

 −1 0 1 5  ∈ M3×3 (R) 2 1 

1  0 Example: The characteristic polynomial of A =   3 1

2 1 2 1

1 2 1 2

 2 3   ∈ 1  0

M4×4 (R) is X 4 − 3X 3 − 11X 2 − 25X − 15. If we sketch the graph of the polynomial function t → t4 − 3t3 − 11t2 − 25t − 15, we see that it has real roots in the neighborhoods of −0.8 and 5.8. (More precisely, they are approximately equal to −0.8062070604 and 5.7448832706.) These are the only real eigenvalues of the matrix A. Example: Let F = GF (3).  1 1  2 0 A=  0 1 1 1

The characteristic polynomial of  1 1 1 0   ∈ M4×4 (F ) 1 0  1 0

equals X 4 + X 3 + 1 = (X + 2)(X 3 + 2X 2 + 2X + 2), and so A has only one eigenvalue, namely 1. 

5 Example: The characteristic polynomial of A =  4 2

4 5 2

 2 2  in 2

M3×3 (Q) is (X − 10)(X − 1)2 and so spec(A) = {1, 10}. The eigenspace   2 of A associated with 10 is Q  2  , while the eigenspace of A 1     −1   −1 associated with 1 is Q  1  ,  0  .   0 2

240


Example: Let F = GF (2) and let A =

0 1 1 1

! ∈ M2×2 (F ).

The characteristic polynomial of A is p(X) = X 2 + X + 1 and, since p(0) = p(1) = 1 we see that spec(A) = ∅. In fact, it is possible to show that for every prime integer p there is a symmetric 2 × 2 matrix A over GF (p) satisfying spec(A) = ∅. Later, we will show that any symmetric matrix over R must have an eigenvalue. Example: Let α be the endomorphism of C2 represented with respect ! 1+i 1 to the canonical basis by the matrix A = ∈ M2×x (C). 1 1−i The characteristic polynomial of A is (X !− 1)2 and so spec(A) = 1 i The eigenspace associated with it is C , which has dimension 1. 1 Therefore α is not diagonalizable. (12.7) Proposition: Let F be a field and let n be a positive integer. If A ∈ Mn×n (F ) has characteristic polynomial p(X) = n i a X , then |A| = (−1)n a0 . i i=0 Proof: We note that a0 = p(0) = |0I − A| = | − A| = (−1)n |A| and so |A| = (−1)n a0 . Any monic polynomial in F [X] of positive degree is the characteristic polynomial of some nsquare matrix over F. To see this, consider a polynomial p(X) = i=0 ai X i , for n > 0. If p(X) is monic, define the companion matrix of p(X) to be the matrix comp(p) ∈ Mn×n (F ) to be the matrix [aij ] given by  1 if i = j + 1 and j < n  −ai−1 if j = n aij = .  0 otherwise Otherwise, define comp(p) to be comp(a−1 n p). (12.8) Proposition: nLet F be a field and let n be a positive integer. If p(X) = i=0 ai X i ∈ F [X] is monic, then p(X) is the characteristic polynomial of comp(p) ∈ Mn×n (F ). Proof: We will proceed by induction on n. For n = 1, the result is immediate. If n = 2 and if p(X) = X 2 + a1 X + a0 , then ! 0 −a0 and so the characteristic polynomial of comp(p) comp(p) = 1 −a1


X a0 is −1 X + a1

241

= p(X) and we are done. Assume now that n > 2 and

the result has been established for n − 1. Then X 0 ... a0 −1 X . . . a 1 mial of comp(p) is .. . . . . . . . 0 . . . −1 X + an−1

the characteristic polyno . By Proposition 11.11, n−1 i this equals X|comp(q)| + a0 (−1)n−1 |B|, where q(X) = i=0 ai+1 X and where B ∈ M(n−1)×(n−1) (F ) is an upper-triangular matrix with diagonal entries all equal to −1. Thus |B| = (−1)n−1 and, by the induction hypothesis, |comp(q)| = q(X). Thus the characteristic polynomial of comp(p) is Xq(X) + a0 = p(X), as desired.

Let F be a field and let n be a positive integer. Every nonsingular matrix P ∈ Mn×n (F ) defines a function ω P from Mn×n (F ) to itself given by ω P : A → P −1 AP. In fact, ω P ∈ Aut(Mn×n (F )), where ω −1 P = ω P −1 . This is an automorphism of F -algebras and, indeed, it can be shown that every automorphism of unital F -algebras in Aut(Mn×n (F )) is of this form. Therefore the set of all automorphisms of the form ω P is a group of automorphisms of Mn×n (F ) and so defines an equivalence relation ∼ by setting A ∼ B if and only if B = P −1 AP. In this case, we say that the matrices A and B are similar. From what we have already seen, two matrices in Mn×n (F ) are similar if and only if they represent the same endomorphism of an n-dimensional vector spacer over F with respect to different bases. One of the problems before us is to decide, given two square matrices of the same size, if they are similar or not. Note that if a matrix A ∈ Mn×n (F ) is similar to O, then it must equal O. Indeed, if P −1 AP = O then A = (P P −1 )A(P P −1 ) = P (P −1 AP )P −1 = P OP −1 = O. 

Example: In  B= 

80 10 −50

130 10 −80

20 10 M3×3 (Q), the matrices A =  10 0 10 10  100 10  are similar, since B = P −1 AP, −60

 10 10  10

and

where P =

 1 2 1  1 0 1  . Thus we note that a symmetric matrix may be similar to 2 3 3 a matrix which is not symmetric.

242


Example: The matrices  1 0 A =  −1 1 −1 0

  0 1 1  and B =  0 2 0

1 1 0

 0 0  2

in M3×3 (Q) are not similar since, were they similar, the matrices A − I and B − I would also be similar, and thus have the same rank. But it is easy to see that the rank of A − I equals 1, while the rank of B − I equals 2. A, B ∈ Mn×n (F )

are similar, it does not   1 0 −1 0  ∈ follow that they commute. For example, let A =  2 3 −1 0 −2   1 0 0 M3×3 (R). Then P =  0 1 0  is nonsingular and so B = P AP −1 = 0 1 1   1 1 −1  2 3 0  is similar to A. However, AB = BA. 1 5 −2 Example:

If matrices

(12.9) Proposition: Let F be a field and let k < n be positive integers. Let A ∈ Mn×n (F ) be a matrix which can be written ! A11 A12 , where A11 ∈ Mk×k (F ) and in block form as A = O A22 A22 ∈ M(n−k)×(n−k) (F ). Then spec(A) = spec(A11 ) ∪ spec(A22 ). Proof: Let c ∈ spec(A) and let v ∈ F n be an eigenvector associated ! v1 , where v1 ∈ F k and v2 ∈ F n−k . Then with c. Write v = v2 A11 v1 + A12 v2 A22 v2

! =

A11 O

A12 A22

!

v1 v2 

! = Av = cv =

cv1 cv2

! .

 0   From this we see immediately that if v2 =  ...  then c ∈ spec(A22 ), 0   0   while if v2 =  ...  then c ∈ spec(A11 ). Therefore spec(A) is contained 0 in spec(A11 ) ∪ spec(A22 ).


Conversely, let c ∈ spec(A11 ) associated with c. Then A

v1 O

!

243

and let v1 ∈ F k be an eigenvector ! ! A11 v1 v1 = =c , proving O O

that c ∈ spec(A). Now assume that d ∈ spec(A22 ) spec(A11 ) and let / spec(A11 ), v2 ∈ F n−k be an eigenvector associated with d. Since d ∈ we know that the matrix B = A11 − dI ∈ Mk×k (F ) is nonsingular. Set   0 ! ! Bv1 + A12 v2 v1  ..  −1 v1 = B A12 (−v2 ). Then (A − dI) = = . , v2 (A22 − dI)v2 0 showing that d ∈ spec(A). Therefore spec(A11 ) ∪ spec(A22 ) ⊆ spec(A), proving equality. 

 6 3   ∈ M4×4 (C). Then 1  3 ! ! 1 1 2 1 ∪ spec −1 1 −4 3

* + √ 1 5 ± i 15 . {1 ± i} ∪ 2

1  −1 Example: Let A =   0 0 spec(A) = spec =

1 5 1 7 0 2 0 −4

(12.10) Proposition: Similar matrices in Mn×n (F ), where F is a field and where n is a positive integer, have identical characteristic polynomials. Proof: If A, B ∈ Mn×n (F ) satisfy B = P −1 AP then |XI−B| = |XI−P −1 AP | = |P −1 (XI−A)P | = |P |−1 |XI−A||P | = |XI−A| as required.

Example: The converse of Proposition 12.10 is false. Indeed, the ! ! 1 1 1 0 matrices and are not similar, despite the fact that 0 1 0 1 both of them have the same characteristic polynomial, (X − 1)2 . Example: If A and B are square matrices over a field F, then we know that the matrices AB and BA are not necessarily equal. ! 1 0 They are also not necessarily similar. For example, if A = and 1 0

244

B=


0 0 1 1

! then AB = O = BA and so AB and BA are not similar.

Nonetheless, by Proposition 12.3, we see that spec(AB) = spec(BA). Proposition 12.10 can be used to facilitate computation, as the following example shows. Example: Let n be a positive integer, let F be a field, and let A = [aij ] ∈ Mn×n (F ) be a symmetric tridiagonal matrix. That is to say, the entries of A satisfy the condition that aij = aji when |i − j| = 1 and aij = 0 when |i − j| > 1. Set p0 (X) = 0 and, for each 1 ≤ k ≤ n, let pk (X) be the characteristic polynomial of the k × k submatrix of A consisting of the first k rows and first k columns of the matrix XI − A ∈ F [X]. Then pn (X) is the characteristic polynomial of A and we have p1 (X) = X − a11 and pk (X) = (X − akk )pk−1 (X) − a2ij pk−2 (X) for each 2 ≤ k ≤ n. This recursion relation allows us to compute the characteristic polynomial of A quickly. Therefore, if A is any symmetric matrix, a good strategy is to try and find a symmetric tridiagonal matrix similar to it and then compute its characteristic polynomial. Let α be an endomorphism of a vector space V finitely generated over a field F and let c ∈ spec(α). The algebraic multiplicity of c is the largest integer k such that (X − c)k divides the characteristic polynomial of α. The geometric multiplicity of c is the dimension of the eigenspace of α associated with c. The geometric multiplicity of c is not greater than its algebraic multiplicity, but these two numbers need not be equal, as the following examples will show. If these two multiplicities are equal, we say that c is a semisimple eigenvalue of α; an eigenvalue which is not semisimple is defective. In particular, if the algebraic multiplicity of c is 1 then the same must be true for its geometric multiplicity. In that case, we say that c is a simple eigenvalue of α. If at least one eigenvalue of α has geometric multiplicity greater than 1, then α is derogatory. ! ! a a+b 2 → Example: If α ∈ End(R ) is defined by α : b b ! 0 then c = 1 is an eigenvalue of α with associated eigenspace R 1 and so the geometric multiplicity of c is 1. On the other hand, α is ! 1 1 represented with respect to the canonical basis by the matrix , 0 1 so its characteristic polynomial is (X − 1)2 , implying that the algebraic multiplicity of c is 2.


245

Example: Let α ∈ End(R3 ) be the endomorphism represented with   2 3 1 4  . The charrespect to the canonical basis by the matrix  3 2 0 0 −1 acteristic polynomial of α is (X − 5)(X + 1)2 and so spec(α) = {−1, 5}, where the algebraic multiplicity of −1 equals 2 and the algebraic multi  −1 plicity of 5 equals 1. The eigenspace associated with −1 is R  1  0   1 and the eigenspace associated with 5 is R  1  . Thus both eigenvalues 0 have geometric multiplicity 1. Hence, 5 is a simple eigenvalue of α whereas −1 is defective. Let n be a positive integer. If α ∈ End(Rn ) is represented with respect to a given basis of Rn by a matrix all entries in which are positive, then Perron, using analytic methods, showed that the eigenvalue of largest absolute value of α is simple and positive, and has an associated eigenvector all entries of which are positive. This result has many important applications in statistics and economics, especially in input-output analysis. It was also used by Thurston in his classification of surface diffeomorphisms in topology. Perron’s results were later extended by Frobenius to certain matrices all entries in which are nonnegative, and later by Karlin to certain endomorphisms of spaces which are not finite-dimensional.3 (12.11) Proposition: Let V be a vector space finitely generated over a field F and let α be an endomorphism of V satisfying the condition that the characteristic polynomial of α

3 Twentieth-century German mathematician Oskar Perron worked in many areas of algebra and geometry. Fellow German mathematician Georg Frobenius is known for his important work in group theory and his work on bilinear forms. He was also the first to consider the rank of a matrix. William Thurston is a contemporary American geometer; contemporary American applied mathematician Samuel Karlin has published extensively in probability and statistics, as well as mathematical biology.

246


is completely reducible. Then α is diagonalizable if and only if every eigenvalue of α is semisimple. Proof: Let spec(α) = {c1 , . . . , ck }. First of all, we will assume that there exists a basis D of V such that ΦDD (α) is a diagonal matrix. For each 1 ≤ j ≤ k, denote by m(j) the number of times that cj appears on k the diagonal of ΦDD (α). Then j=1 m(j) = n and by Proposition 12.4, we know that for each 1 ≤ j ≤ k there exists a subset of D, having m(j) elements, which is a basis for the eigenspace of α associated with cj . k m(j) and so Moreover, the characteristic polynomial of α is j=1 (X − cj ) m(j) equals both the algebraic multiplicity and the geometric multiplicity of cj for each 1 ≤ j ≤ k, proving that each such cj is semisimple. Conversely, assume that each cj is semisimple, and for each 1 ≤ j ≤ k let m(j) be the algebraic (and geometric) multiplicity of cj . Let Dj be k a basis for the eigenspace of α associated with cj , and let D = j=1 Dj . Then D is a linearly-independent subset of V having n elements, and so is a basis of V over F. The result then follows from Proposition 7.5. Example: The condition in Proposition 12.11 that the characteristic polynomial of α be completely reducible is essential. To see this, consider the endomorphism α of R3 represented with respect to the canonical   0 1 0 basis by the matrix A =  −1 0 0  . The characteristic polynomial 0 0 1 of α is (X − 1)(X 2 + 1) ∈ R[X] and so spec(α) = {1}, where 1 is a simple eigenvalue of α and so it is surely semisimple. The eigenspace of   1 α associated with this eigenvalue is R  0  and so its dimension is 1. 0 Hence α is not diagonalizable. Example: Consider the endomorphism α of R3 represented with   −1 −1 −2 8 −11 −8  and let respect to the canonical basis by the matrix  −10 11 7 β be the endomorphism of R3 represented with respect to the canonical   1 −4 −4 basis by the matrix  8 −11 −8  . These two endomorphisms have −8 8 5 the same characteristic polynomial X 3 + 5X 2 + 3X − 9 = (X − 1)(X + 3)2 . Thus the algebraic multiplicity of the eigenvalue 1 equals 1 and the


247

algebraic multiplicity of the eigenvalue −3 equals 2. But for α, the geometric multiplicity of −2 equals 1, so α is not diagonalizable. On the other hand, for β the geometric multiplicity of −2 equals 2, and so β is diagonalizable. Let F be a field and let (K, •) be an associative unital F -algebra. If k k v ∈ K and if p(X) = i=0 ci X i ∈ F [X], then p(v) = i=0 ci v i ∈ K. For any polynomial q(X) ∈ F [X] we have p(v) • q(v) = q(v) • p(v). In particular, v • p(v) = p(v) • v. It is clear that Ann(v) = {p(X) ∈ F [X] | p(v) = 0K } is a subspace of F [X]. If p(v) = 0K , we say that v annihilates the polynomial p(X). In particular, we note that all of the above is true for the associative unital F -algebra Mn×n (F ), where n is a positive integer. We note that if A ∼ B in Mn×n (F ) then there is a nonsingular matrix P such that B = P −1 AP and so p(B) = P −1 p(A)P so that if p(A) = O then p(B) = O. Thus we see that Ann(A) = Ann(B) whenever the matrices A and B are similar. ! 2 1 Example: Let A = ∈ M2×2 (R) and let p(X) = X 2 −X +2 ∈ 1 0 ! 5 1 . If q(X) = X 2 − 2X − 1 R[X]. Then p(A) = A2 − A + 2I = 1 3 then q(A) = O so q(X) ∈ Ann(A). (12.12) Proposition: Let F be a field and let (K, •) be an associative F -algebra of finite dimension over F. Then Ann(v) is nontrivial for each v ∈ K. Proof: Let dim(V ) = n. If v ∈ K then v 0 , v 1 , . . . , v n must be linearly dependent there exist scalars a0 , . . . , an , not all equal to n and so i v = 0K . In other words, there exists a nonzero 0, such that i i=0 a n i in Ann(v). polynomial p(X) = i=0 ai X We now show why one cannot define “three-dimensional complex numbers”. (12.13) Proposition: If n is an odd integer greater than 1 then there is no way of defining on Rn the structure of an R-algebra which is also a field. Proof: Assume that we can define an operation on Rn (which we will denote by concatenation) which turns it into an R-algebra which is also a field, and let v1 be the identity element for this operation. Then V = Rv1 since dim(V ) > 1. Pick an element y ∈ V Rv1 and let α ∈ End(V ) be

248


given by α : v → yv, which is represented with respect to the canonical basis of Rn by a matrix A. The characteristic polynomial p(X) of A belongs to R[X] and has odd degree; therefore it has a root c in R. Thus p(X) = (X − c)k q(X) for some k ≥ 1 and some q(X) ∈ R[X] satisfying q(c) = 0. Let β ∈ End(V ) be given by β : v → (y −cv1 )k v. Then β = σ 0 since y ∈ / Rv1 and 0V = q(c) = q(cv1 ). But then (y − cv1 )k q(cv1 ) = 0V , contradicting Proposition 2.3(12). Let F be a field and let (K, •) be an associative unital F -algebra. If v ∈ K satisfies the condition thatAnn(v) is nontrivial then Ann(v) n i of minimal degree. This must contain a polynomial p(X) = i=0 ai X means, in particular, that an = 0 and so the monic polynomial a−1 n p(X) also belongs to Ann(v). We claim that it is the unique monic polynomial of minimal degree in Ann(v). Indeed, if q(X) is a monic polynomial of degree n belonging to Ann(v) not equal to a−1 n p(X), then r(X) = q(X) − a−1 n p(X) ∈ Ann(v). But deg(r) < n, contradicting the minimality of the degree n of p(X). Thus we see that Ann(v), if nonempty, contains a unique monic polynomial of minimal positive degree, which we call the minimal polynomial of v over F and denote by mv (X). In particular, if F is a field and if n is a positive integer, then any matrix A ∈ Mn×n (F ) has a minimal polynomial, which we denote by mA (X). If A and B are similar matrices, then mA (X) = mB (X). Similarly, if V is a vector space finitely generated over a field F, and if α ∈ End(V ) then α has a minimal polynomial mα (X), and this equals the minimal polynomial of ΦDD (α) for any basis D of V. Example: Let (K, •) be an associative unital entire R-algebra. Assume that v ∈ K has a minimal polynomial mv (X) ∈ R[X]. By the Proposition t 4.4, we know that mv (X) = i=1 pi (X), where the pi (X) are irreducible t polynomials of degree at most 2. But then i=1 pi (v) = 0K and, since K is entire, there is some index h such that ph (v) = 0K . By minimality, this means that mv (X) = ph (X). We thus conclude that any element of v having a minimal polynomial has one of degree at most 2. (12.14) Proposition: Let F be a field and let (K, •) be an associative F -algebra of finite dimension over F. If v ∈ K satisfies the condition that Ann(v) is nontrivial and if p(X) ∈ Ann(v), then there is a polynomial q(X) ∈ F [X] satisfying p(X) = mv (X)q(X).

Proof: If p(X) is the 0-polynomial, pick u(X) to be the 0-polynomial and we are done. Therefore assume that deg(p) > 0. From Proposition 4.2, we know that we can write p(X) = mv (X)q(X) + r(X), where q(X), r(X) ∈ F [X], with deg(r) < deg(mv ). Since p(v) = 0K we


249

see that 0K = mv (v) • q(v) + r(v) = r(v). Since deg(v) < deg(mA ), we must have deg(v) = −∞ and so p(X) = mv (X)q(X). (12.15) Proposition: Let F be a field and let (K, •) be an associative unital F -algebra with multiplicative identity e. If n v ∈ K has a minimal polynomial mv (X) = i=0 ai X i then: (1) v is a unit of K if and only if a0 = 0; and (2) If v is a unit of K then v −1 = g(v), where g(X) =

n

i−1 (−a−1 ∈ F [X]. 0 ai )X

i=1

Proof: If a0 = 0 then mv (v) = 0K implies that n n −1 −1 i i−1 e = a0 − • v = g(v) • v = v • g(v) ai v = a0 − ai v i=1

i=1

and so v is a unit and v −1 = g(v). Conversely, assume( that v is a) n i−1 have 0 = m (v) = v • unit. Had we a0 = 0, we would V v i=1 ai v n n −1 i−1 i−1 and so 0K = v mv (v) = i=1 ai v . Thus ∈ Ann(v), i=1 ai X contradicting the minimality of the degree mv (X). Hence a0 = 0. It is important to note that the minimal polynomial of a matrix over a field need not equal its characteristic polynomial. For example, if we consider I ∈ Mn×n (F ) for any field F and any integer n > 1, then the characteristic polynomial of I is (X −1)n whereas its minimal polynomial is X − 1. Example: Let F be a field. The matrix A =

1 0

0 0

! ∈ M2×2 (F )

annihilates the polynomial X(X − 1), and this is in fact its minimal polynomial. It is also the characteristic polynomial of A. Thus we see that the minimal polynomial of a matrix does not have to be irreducible. Notice too that the rank of A equals 1, but the degree of its minimal polynomial is 2. Thus the degree of the minimal polynomial of a matrix may be larger than its rank. 

Example:

Let F

1 be a field. The matrix A =  0 0

0 0 0

 0 0  ∈ 0

M3×3 (F ) annihilates the polynomial X(X − 1), and this is in fact its minimal polynomial. The characteristic polynomial of A is X 2 (X − 1).

250




1 Example: One can check that  0 0

0 3 0

  0 1 0 ,  0 3 0

0 1 0

 0 0  ∈ M3×3 (Q) 3

are not similar, but they both have the same minimal polynomial, namely (X − 1)(X − 3). Example: Proposition 12.15 can be used to calculate the inverse of a nonsingular matrix, though it is rarely the most efficient method of do  2 −2 4 3 2  has minimal ing so. For example, the matrix A =  2 −1 1 −1 2 1 A − 4A + 7I = polynomial X 3 − 4X 2 + 7X − 10 = 0 so A−1 = 10   −5 2 −16 1  0 2 4 . 10 5 0 10 (12.16) Proposition (Cayley-Hamilton Theorem): Let F be a field and let n be a positive integer. Then every matrix in Mn×n (F ) annihilates its characteristic polynomial. Proof: Let A be a matrix in Mn×n (F ) having minimal polynomial n−1 p(X) = X n + i=0 ai X i . Let us look at the matrix [gij (X)] = adj(XI − A) ∈ Mn×n (F [X]), where each gij (X) is a polynomial at most n − 1. Then we can n of degree n−i B X , where the Bi are matrices write this matrix in the form i=1 i in Mn×n (F ). Moreover, we know that p(X)I

|XI − A|I = (XI − A) adj(XI − A) " n # n−i = (XI − A) . Bi X

=

i=1

Equating coefficients of the various powers of X, we thus see B1 B2 − AB1 B3 − AB2 Bn − ABn−1 −ABn

= I = an−1 I = an−2 I ... = a1 I = a0 I


251

For 1 ≤ h ≤ n, multiply both sides of the hth equation in the above list on the left by An+1−h and then sum both sides, to obtain O = p(A), as desired. In particular, we conclude from Proposition 12.14 and Proposition 12.16 that the minimal polynomial of any n × n matrix over a field divides its characteristic polynomial and so the degree of the minimal polynomial is at most n. Let V be a vector space finitely generated over a field F and let σ 0 = α ∈ End(V ). In Proposition 12.4 we saw that α is diagonalizable if and only if that basis is composed of eigenvectors of V. Moreover, if spec(α) = {c1 , . . . , ck } and if, for each 1 ≤ i ≤ k, we denote the eigenspace of α associated with ci by Wi , then for each 1 ≤ i ≤ k we have a projection π i ∈ End(V ) satisfying the following conditions: (1) im(π i ) = Wi ; (2) π 1 + . . . + π n = σ 1 ; (3) π i π j = σ 0 whenever i = j; (4) α = c1 π 1 + . . . + ck π k . For each 1 ≤ h ≤ k, let ph (X) be the hth Lagrange interpolation polynomial determined by c1 , . . . , ck . Then we can check that π h = ph (α) for each h, since ph (X)(X − ch ) is just a scalar multiple of the minimal polynomial of α. Is it possible to simultaneously diagonalize two distinct endomorphisms of V ? Indeed, let V be a vector space finitely generated over a field F and let α and β be distinct elements of End(V ) {σ 0 }. There exists a basis D of V such that both ΦDD (α) and ΦDD (β) are diagonal matrices if and only if the elements of D are eigenvectors of α as well as of β. Suppose that we have in hand such a basis D = {u1 , . . . , uk }. Since diagonal matrices commute with each other, we see that ΦDD (αβ) = ΦDD (α)ΦDD (β) = ΦDD (β)ΦDD (α) = ΦDD (βα) and so αβ = βα. Therefore a necessary condition for both endomorphisms of V to be represented by diagonal matrices with respect to the same basis is that they form a commuting pair. We also note that if D is be a basis for a vector space V over a field F . Then the set of all endomorphisms α of V satisfying the condition that ΦDD (α) is a diagonal matrix is a subspace of End(V ). Indeed, this is an immediate consequence of the fact that the set of all diagonal n × n matrices is a subspace of Mn×n (F ). (12.17) Proposition: Let V be a vector space over a field F and let (α, β) be a commuting pair of endomorphisms of V. Then p(α)q(β) = q(β)p(α) for any p(X), q(X) ∈ F [X].

252


Proof: nInitially, we will consider the special case of q(X) = X. If p(X) = i=0 ai X i then βα2 = (βα)α = (αβ)α = α(βα) = α(αβ) = α2 β, and by induction we similarly have βαk = αk β for every positive integer k. Therefore # # " n " n n n i i i i ai α = ai βα = ai α β = ai α β = p(α)β. βp(α) = β i=0

i=0

i=0

i=0

Now a proof similar to the first part shows that p(α)β k = β k p(α) for every positive integer k and hence, by a proof similar to the second part, we get p(α)q(β) = q(β)p(α) for any p(X), q(X) ∈ F [X]. As a consequence of this we note that if α, β ∈ End(V ) are commuting projections then (αβ)2 = (αβ)(αβ) = α(βα)β = α(αβ)β = α2 β 2 = αβ and so αβ is a projection as well. (12.18) Proposition: Let V be a vector space finitely generated over a field F and let α, β ∈ End(V ) be diagonalizable endomorphisms of V. Then there exists a basis of V relative to which both α and β can be represented by diagonal matrices if and only if αβ = βα. Proof: We have already noted that if α and β can both be represented by diagonal matrices with respect to a given basis of V then we must have αβ = βα. Conversely, assume that α and β are diagonalizable endomorphisms of V satisfying αβ = βα. Then, as we have already seen, there exist distinct scalars c1 , . . . , ck and projections π 1 , . . . , π k ∈ End(V ) such that π 1 + . . . + π k = σ 1 , π i π j = σ 0 for i = j, and c1 π 1 + . . . + ck π k = α. Similarly, there exist scalars d1 , . . . , dt and projections η 1 , . . . , η k ∈ End(V ) such that η 1 + . . . + η k = σ 1 , η i η j = σ 0 for i = j, and d1 η 1 + . . . + dk η k = β. Therefore  # t " k k t ci π i  ηj  = ci π i η j α = ασ 1 = i=1

and

j=1

i=1 j=1

"  # t k t k β = βσ 1 =  dj η j  πi = dj η j π i . j=1

i=1

j=1 i=1

Since we saw that, for each 1 ≤ i ≤ k we have π i = pi (α) for some pi (X) ∈ F [X] and similarly for each 1 ≤ j ≤ t we have η j = qj (β) for some qj (X) ∈ F [X], we conclude that π i η j = η j π i for each such i and j. Call this common value θij . By the comments after Proposition 12.17, we see that θij is also a projection in End(V ).


253

We note that θij θhm = π i η j π h η m = π i π h η j η m and this equals σ 0 when i = j or h = m. We also note that  # t " k k t θij = πi  ηj  = σ1 . i=1 j=1

i=1

j=1

Thus we have shown that α and β are simultaneously diagonalizable, using those projections θij which are nonzero (as some of them may be). Algorithms for the computation of the eigenvalues and eigenvectors of a given matrix are usually very complicated, especially if speed of computation is a major consideration. Therefore, we shall not go into the description of such algorithms in detail. As a rule of thumb, it is best to try to compute eigenvectors directly, and not through finding roots of the characteristic polynomial, since small errors in the computation of eigenvalues may often lead to large errors in the computation of the corresponding eigenvectors. For matrices over R, there are often reasonably efficient iterative methods to find at least some of the eigenvectors. We will bring here one example to find an eigenvector associated with the real eigenvalue of a matrix over R having greatest absolute value, under assumption that such an eigenvalue indeed exists. The algorithm is based on the observation that if c is an eigenvalue of a matrix A ∈ Mn×n (R) then ck is an eigenvalue of Ak . Therefore, if k is sufficiently large, the matrix A(Ak ) is approximately equal to cAk . Therefore, if we select an arbitrary vector v (0) ∈ Rn and successively define vectors v (1) , v (2) , . . . by setting v (i+1) = Av (i) for each i ≥ 0, then Av (k) = Ak+1 v (0) and this is roughly equal to cv (k) . Therefore, if the conditions are amenable (and we will not go into the precise conditions necessary for this to happen), the vector v (k) is a reasonable approximation to an eigenvector of A associated with c. Of course, we must always remember that repeated computations lead to accumulating roundoff and truncation errors; one way of combating these is to divide each entry in v (i) by the absolute value of the largest entry, and use this “normalized” vector in the next iteration4 .

4

Of the many numerical analysts who studied computational methods for finding eigenvalues, one of the most important is the British mathematician James H. Wilkinson, a former assistant of Alan Turing and one of the major early innovators in numerical linear algebra. The iteration algorithm given here

254


! 5 1 Example: Consider A = ∈ M2×2 (R) and let us pick −3 1 ! 1 then v (0) = 1 ! ! 1 6 (0) (1) Av = ; and so we will take v = −2 − 31 Av

(1)

1 = 3

14 −10

1 7

30 −26

Av (2) =

Av

(3)

1 = 13

Av (4) =

1 31

62 −58

! and so we will take v

(2)

=

1

126 −122

and so we will take v

!

1

;

− 15 13

! (4)

;

− 57

! and so we will take v (3) =

!

=

! and so we will take v (5) =

It seems that this sequence of vectors is converging to

1

! ;

− 29 31 1

!

− 61 63 1 −1

. ! and,

indeed, one can check that this is an eigenvector of A associated with the eigenvalue 4. Example: Let n be a positive integer and let A ∈ Mn×n (R) be a T matrix of the form [cB + (1 − c)D] , where B ∈ Mn×n (R) is a Markov     1 d1     matrix, c ∈ R satisfies 0 ≤ c ≤ 1, and D =  ...  ∧  ...  for dn 1 nonnegative real numbers di satisfying i=1 di = 1. Such matrices have been called Google matrices since they are needed for the PageTM to compute Rank algorithm used by the internet search engine Google an estimate of web-page importance for ranking search results (for these purposes, a typical value for c is 0.85). The value of n can be very large, often far larger than 109 . One can show that the eigenvalues e1 , . . . , en of such a matrix satisfy 1 = |e1 | ≥ |e2 | ≥ . . . ≥ |en | ≥ 0 and so the power method mentioned above can (and is) used by Google to rapidly compute an eigenvector associated to e1 . Recently, Stanford University researchers Taher Haveliwala and Sepandar Kamvar have shown that for any Google matrix, |e2 | ≤ c, with n

was first studied in the 1920’s by the Austrian applied mathematician Richard von Mises, who later emigrated to the United States.


255

equality happening under conditions that hold in the case of those matrices arising in this particular application. Eigenvectors corresponding to this second eigenvalue can be used to detect and combat link spamming on the internet. One can also consider a generalization of the eigenvalue problem: given endomorphisms α and β of a vector space V, find all scalars c such that cβ − α is not monic. Problems of this sort arise naturally, for example, in plasma physics and in the design of control systems. When β is an automorphism, as is usually the case, this can be reduced to the usual eigenvalue problem for the endomorphism β −1 α, but there are sometimes reasons for not wanting to do so. For example, even if both α and β are represented with respect to a given basis by symmetric matrices, the matrix representing β −1 α may not be symmetric. Therefore, some specialized algorithms have been developed to find solutions of the generalized eigenvalue problem directly.

Exercises Exercise 667 Find the characteristic polynomial of the matrix   3 2 2  1 4 1  ∈ M3×3 (R). 2 −4 −1 Exercise 668 Find the characteristic polynomial of the matrix   1 3 0 0 0  0 1 0 0 0     0 0 1 0 0  ∈ M5×5 (R).    0 0 2 2 0  0 0 0 0 2 Exercise 669 Let a, b, c ∈ R. Find the characteristic polynomial of the   0 0 0 a  a 0 0 b   matrix   0 b 0 c  ∈ M4×4 (R). 0 0 c 0 Exercise 670 Let n be a positive integer and let A ∈ Mn×n (Q). Let c1 , . . . , cn be the list of (not necessarily distinct) eigenvalues of A, conn n sidered as a matrix in Mn×n (C). Show that ci are i=1 ci and i=1 rational numbers.

256


Exercise 671 Let F be a field, let n be a positive integer, and let A, B ∈ Mn×n (F ). Assume that A and B have the same characteristic polynomial p(X) ∈ F [X]. Is it necessarily true that p(X) is the characteristic polynomial of AB? Exercise 672 Find infinitely-many matrices in M3×3 (R), all of which have characteristic polynomial X(X − 1)(X − 2). Exercise 673 Let n be a positive integer. Show that every matrix A ∈ Mn×n (R) can be written as the sum of two nonsingular matrices. Exercise 674 Let F = GF (3) and let n be a positive integer. Let D = [dij ] ∈ Mn×n (F ) be a nonsingular diagonal matrix and let A ∈ Mn×n (F ). Show that 1 ∈ / spec(DA) if and only if D − A is nonsingular. Exercise 675 Let F be a field of characteristic other than 2. For each positive integer n, let Tn be the set of all diagonal matrices in Mn×n (R) the diagonal entries of which belong to {−1, 1}. For any A ∈ Mn×n (R), / spec(DA). show that there exists a matrix D ∈ Tn satisfying 1 ∈ Exercise 676 Let n be a positive integer  a0  .. be the function defined by α : A →  .

and let α : Mn×n (C) → Cn  n−1   , where X n + i=0 ai X i

an−1 is the characteristic polynomial of A. Is α a linear transformation? Exercise 677 Let α be the endomorphism of R3 defined by     a a−b α :  b  →  a + 2b + c  . c −2a + b − c Find the eigenvalues of α and, for each eigenvalue, find the associated eigenspace. Exercise 678 Let A is a nonempty set and let V be the collection of all subsets of A, which is a vector space over GF (2). Let B be a fixed subset of A and let α : V → V be the endomorphism defined by α : Y → Y ∩ B. Find the eigenvalues of α and, for each eigenvalue, find the associated eigenspace. Exercise 679 Let α be the endomorphism of R4 defined by     a b+c  b   c     α:  c  →  0  . d 0


257

Find the eigenvalues of α. Do there exist two-dimensional subspaces W and Y of R4 , both invariant under α, such that R4 = W ⊕ Y ? Exercise 680 Let V be a vector space finitely generated over a field F and let α be an endomorphism of V having an eigenvalue c. For any p(X) ∈ F [X], show that p(c) is an eigenvalue of p(α). Exercise 681 Let V be the vector space of all functions in RR which are infinitely differentiable and let α : V → V be the endomorphism of V defined by α : f → f . If n is an integer, show that the function f : x → sin(nx) is an eigenvector of α2 and find the associated eigenvalue. Exercise 682 Let F be a field and let V = F (Z) . Let α be the endomorphism of V defined by α(f ) : i → f (i + 1) for all i ∈ Z. Show that spec(α) = ∅. Exercise 683 Let V be the vector space composed of all polynomial functions from R to itself, let a ∈ R, and let α be the endomorphism of V defined by α(p) : x → (x − a) [p (x) + p (a)] − 2 [p(x) − p(a)] , where p denotes the derivative of p. Find the eigenvalues of α and for each such eigenvalue, find the associated eigenspace. Exercise 684 Let α be the endomorphism of M2×2 (R) defined by ! ! a b d −b α: → . Find the eigenvalues of α and for each c d −c a such eigenvalue, find the associated eigenspace. Exercise 685 Let V be a vector space over Q and let α ∈ End(V ) be a projection. Show that spec(α) ⊆ {0, 1}. Exercise 686 Let V be a vector space of dimension n > 0 over a field F. Let α be an endomorphism of V for which there exists a set A of n + 1 distinct eigenvectors satisfying the condition that every subset of A of size n is a basis for V. Show that all of the eigenvectors in V are associated with the same eigenvalue c of α and that α = cσ 1 .   a b 0 Exercise 687 For a, b ∈ R, let A =  b a b  ∈ M3×3 (R). Find 0 b a the eigenvalues of A. ! a b Exercise 688 Let A ∈ M2×2 (R) be a matrix of the form , c a where a > 0 and bc > 0. Show that A has two distinct eigenvalues in R.

258


 Exercise 689 Find the eigenvalues of the matrix

5 6  −1 0 2 2

 −3 1  ∈ −1

M3×3 (R) and, for each such eigenvalue, find the associated eigenspace.   0 2 1 0 3  ∈ Exercise 690 Find the eigenvalues of the matrix  −2 −1 −3 0 M3×3 (C) and, for each such eigenvalue, find the associated eigenspace. Exercise 691 Let W be the subspace of R∞ consisting of all convergent sequences and let α be the endomorphism of W defined by * + lim ai − a1 , lim ai − a2 , . . . . α : [a1 , a2 , . . .] → i→∞

i→∞

Find all eigenvalues of α and, for each eigenvalue, find the corresponding eigenspace.   1 −1 1 0 0  in Exercise 692 Find the eigenvalues of the matrix  1 0 1 0 M3×3 (C) and, for each such eigenvalue, find the associated eigenspace. Exercise 693 Does there exist a real number a such that   1 −1 0 a −1  = {−2, −1, 0}? spec  0 −6 11 −5 Exercise 694 Let α be an endomorphism of a vector space V over a field F and let v and w be eigenvectors of α. If v +w = 0V , show that v + w is an eigenvector of α if and only if both v and w correspond to the same eigenvalue.   1 0 a a  has three disExercise 695 Show that the matrix A =  a a a 0 −1 tinct eigenvalues for any real number a. Exercise 696 Let n be a positive integer and let t be a nonzero real number. Let A ∈ Mn×n (R) be the matrix all of the entries of which equal t. Find the eigenvalues of A and, for each such eigenvalue, find the associated eigenspace. Exercise 697 Let n be a positive integer and let F be a field. Let A be a nonsingular matrix in Mn×n (F ). Given the eigenvalues of A, find the eigenvalues of A−1 .


259

Exercise 698 Let n be a positive integer and let F be a field. Let A = [aij ] ∈ Mn×n (F ), and let c ∈ spec(A). If b, d ∈ F, show that bc + d ∈ spec(bA + dI). ! a b Exercise 699 Let A = ∈ M2×2 (R). If t ∈ R is a root of the c d ! 1 is an eigenvector polynomial bX 2 +(a−d)X −c ∈ R[X], show that t of A associated with the eigenvalue a + bt. Exercise 700 Let A ∈ M2×2 (C) be a matrix having two distinct eigenvalues. Show that there are precisely four distinct matrices B ∈ M2×2 (C) satisfying B 2 = A.   a 0 0 Exercise 701 Find all a ∈ R such that  2a 2a 2a  has a unique 0 0 a eigenvalue. Exercise 702  a matrix  −1 0

Find a real number a such that the only eigenvalue of the  1 0 0 −1  ∈ M3×3 (R) is 0. 1 −a

Exercise 703 For 1 ≤ i ≤ 3 and 2 ≤ j ≤ 3, find a real number aij       1 1 1 such that  −1  ,  0  , and  1  are all eigenvectors of the 0 −1 1   1 a12 a13 matrix  1 a22 a23  ∈ M3×3 (R). 1 a32 a33 Exercise 704 Let 0 = r ∈ C and let n and m be positive integers. Let A = [aij ] ∈ Mn×n (C) be given and let B = [bij ] ∈ Mn×n (C) be the matrix defined by bij = rm+i−j aij for all 1 ≤ i, j ≤ n. Show that if d ∈ C is an eigenvalue of A then rm d is an eigenvalue of B. Exercise 705 Let n be a positive integer and let F be a field. A matrix A ∈ Mn×n (F ) is a magic matrix if and only if there exists a scalar c ∈ F such that the sum of the entries in each row and each column is c. Characterize magic matrices in terms of their eigenvalues. ! a−1 −1 ∈ Exercise 706 Show that all matrices of the form a2 − a + 1 −a M2×2 (C) have the same eigenvalues.

260


Exercise 707 Let A ∈ M2×2 (C) be a matrix having distinct eigenvalues a = b. Show that, for all n > 0, An =

bn an (A − bI) + (A − aI). a−b b−a

Exercise 708 Let A ∈ M2×2 (C) be a matrix having a unique eigenvalue c. Show that An = cn−1 [nA − (n − 1)cI] for all n > 0. Exercise 709 Let n be a positive integer and let A ∈ Mn×n (C). Show that every eigenvector of A is also an eigenvector of adj(A). Exercise 710 Let n be a positive integer. Let G be the set of all matrices A ∈ Mn×n (C) satisfying the condition that Cn has a basis composed of eigenvectors of A. Is G closed under taking sums? Is it closed under taking products? Exercise 711 Let p(X) ∈ C[X] and let A ∈ Mn×n (C) for some positive integer n. Calculate the determinant of the matrix p(A) using the eigenvalues of A. ! 1 − a + a2 1 − a ∈ Exercise 712 Let −1 = a ∈ R and let A = a a − a2 n M2×2 (R). Calculate A for all n ≥ 1. Exercise 713 Let n be a positive integer. Given a matrix A ∈ Mn×n (Q), find infinitely-many distinct matrices having the same eigenvalues as A. Exercise 714 Let c ∈ R. Find the  1 0 0  0 0 c A=  0 −c 0 0 0 0

spectral radius of  0 0   ∈ M4×4 (C). 0  0

Exercise 715 Let A ∈ Mn×n (R) be a matrix all entries in which are positive and let c be a positive real number greater than the spectral radius of A. Show that |cI − A| > 0. Exercise 716 Let n be a positive integer. Show that 1 is an eigenvalue of any Markov matrix in Mn×n (R). Exercise 717 Let n be apositive integer. Let A = [aij ] ∈ Mn×n (R) n satisfy the condition that j=1 |aij | ≤ 1 for all 1 ≤ j ≤ n. Show that |c| ≤ 1 for all c ∈ spec(A). Exercise 718 Let n be a positive integer and let F be a field. Let A = [aij ] ∈ Mn×n (F ) be a matrix satisfying the condition that the sum of


261



 b1   the entries in each row equals 1. Let 1 = c ∈ spec(A) and let  ...  bn n b = 0. be an eigenvalue of A associated with c. Show that j j=1 Exercise 719 Give an example of a matrix A ∈ M2×2 (R) satisfying the condition that spec(A) = ∅ but spec(A4 ) = ∅. Exercise 720 Find an example of matrices A, B ∈ M2×2 (R) satisfying the condition that every element of spec(A) ∪ spec(B) is positive but every element of spec(AB) is negative. Exercise 721 Find a polynomial p(X) ∈ C[X] of degree 2 satisfying ! 1−a 1 , the condition that all matrices in M2×2 (C) of the form p(a) a for a ∈ C, have the same characteristic polynomial. Exercise 722 Let F be a field and let n be an even positive integer. Let A, B ∈ Mn×n (F ) be matrices satisfying A = B 2 . Let p(X) be the characteristic polynomial of A and let q(X) be the characteristic polynomial of B. Show that p(X 2 ) = q(X)q(−X). Exercise 723 Let F be a field. Characterize the matrices in M2×2 (F ) having the property that their characteristic polynomial is not equal to their minimal polynomial. Exercise 724 Let (K, •) be an associative unital F -algebra, let v ∈ K, and let α : K → K be a homomorphism of F -algebras. Show that Ann(v) ⊆ Ann(α(v)). ! ! 1 2 4 2 Exercise 725 Are the matrices and in M2×2 (R) 3 4 3 1 similar?     1 i 0 1+i 7 2 1 9  Exercise 726 Are the matrices  i 2 −1  and  0 0 i 1 0 0 2−i in M3×3 (C) similar? Exercise 727 Let n be a positive integer and let A, B ∈ Mn×n (R). Show that if A and B are similar when considered as elements of Mn×n (C), they are also similar in Mn×n (R). Exercise 728   Find a diagonal matrix in M3×3 (R) similar to the matrix 1 0 1  0 1 0 . 1 0 1

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Exercise 729   Find a diagonal matrix in M3×3 (R) similar to the matrix 0 0 1  0 0 0 . 1 0 0 Exercise 730 Is there a diagonal matrix in M3×3 (R) similar to the   8 3 −3 3 ? matrix  −6 −1 12 6 −4 Exercise 731 in the subspace of M2×2 (R) gen Show!that every matrix !0 1 1 0 erated by , is similar to a diagonal matrix. 1 0 0 −1 

0 Exercise 732 Determine if the matrices  0 0 in M3×3 (GF (5)) are similar.

1 0 0

  0 0 1  and  1 0 0

0 0 1

 0 0  0

Exercise 733 Is there a diagonal matrix in M3×3 (R) similar to the   1 −1 1 1 2 ? matrix  −2 −2 −1 4 

1 Exercise 734 Let A =  0 0

 0 1  ∈ M3×3 (R). Find a nonsingular 1

0 1 1

matrix P ∈ M3×3 (R) such that P −1 AP is a diagonal matrix. Exercise 735 Show that the matrix A =

1 i i −1

! ∈ M2×2 (C) is not

similar to a diagonal matrix. 

  1 −1 0 2 2 5  and  −1 Exercise 736 Are the matrices  0 0 0 3 0 M3×3 (Q) similar?

0 4 3

 0 0  in 7

Exercise 737 Let k and n be positive integers and let F be a field. ! AB O Let A ∈ Mk×n (F ) and B ∈ Mn×k (F ). Is the matrix B O ! O O similar to the matrix ? B BA


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

 a 1 0 Exercise 738 Let F be a field and let A =  0 a 1  ∈ M3×3 (F ). For 0 0 a   p(a) p (a) 12 p (a) p(a) p (a)  , where any p(X) ∈ F [X], show that p(A) =  0 0 0 p(a) p (X) denotes the formal derivative of the polynomial p(X) and p (X) is the formal derivative of p (X). Exercise 739 Find the characteristic and minimal polynomials of the ma  7 4 −4 trix  4 −8 −1  ∈ M3×3 (R). −4 −1 −8 Exercise 740 Let n be a positive integer. Let V be the vector space over R consisting of all polynomial functions from R to itself having degree at most n. Let α be the endomorphism of V which assigns to each f ∈ V its derivative, and let A be a matrix representing α with respect to some basis of V. Find the minimal polynomial of A. Exercise 741 Find six distinct matrices in M2×2 (R) which annihilate the polynomial X 2 − 1. Exercise 742 Let n be a positive integer and let c be an element of a field F. Find a matrix A ∈ Mn×n (F ) having minimal polynomial (X − c)n . Exercise 743 Use the Cayley-Hamilton Theorem to find the inverse of   5 1 −1  −6 0 2  ∈ M3×3 (R). 0 0 2 Exercise 744 Let n be a positive integer and let A ∈ Mn×n (F ) be a matrix of rank h. Show that the degree of the minimal polynomial of A is at most h + 1. Exercise 745 Let n be a positive integer and let F be a field. Show that a matrix A ∈ Mn×n (F ) is nonsingular if and only if mA (0) = 0.  Exercise 746 Find the eigenvalues of the matrix

0  0   0 1

M4×4 (Q) and determine the algebraic multiplicity of each.

0 0 1 1

1 1 0 0

 1 0   ∈ 0  0

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

0 1 Exercise 747 Find the minimal polynomial of the matrix  0 0 1 3 in M3×3 (R). Exercise 748 Let α and β be the endomorphisms of Q4  1 0  0 1 with respect to the canonical basis by the matrices   1 0 0 1   4 −1 −1 0  −1 4 0 −1   respectively. Does there exist a and   1 0 2 −1  0 1 −1 2

 0 1  −3

represented  −1 0 0 −1   −1 0  0 −1 basis of Q4

with respect to which both of them can be represented by diagonal matrices? Exercise 749 Let α be the endomorphisms of R3 represented with   −6 2 −5 4 −2  . Calculate respect to the canonical basis by the matrix  4 10 −3 8 the algebraic and geometric multiplicities of each of the eigenvalues of α. Exercise 750 Let A = [aij ] ∈ Mn×n (C) be a symmetric tridiagonal matrix having an eigenvalue c with algebraic multiplicity k. Show that ai−1,i = 0 for at least k − 1 values of i. Exercise 751 Let α be the endomorphisms of R3 represented with   −8 −13 −14 −5 −8  . Does respect to the canonical basis by the matrix  −6 14 17 21 there exist a basis of a diagonal matrix?

R3 with respect to which α can be represented by 

 17 −8 −12 14  46 −22 −35 41   ∈ M4×4 (Q). Find the Exercise 752 Let A =   −2 1 4 −4  4 −2 −2 3 minimal polynomial A. ! cos(t) sin(t) cos2 (t) ∈ Exercise 753 For each t ∈ R, set A(t) = cos(t) sin(t) sin2 (t) M2×2 (R). Show that all of these matrices have the same characteristic and minimal polynomials.


265

Exercise 754 Let a, b, c ∈ C. Find a necessary and sufficient condition   2 0 0 for the minimal polynomial of  a 2 0  ∈ M3×3 (C) to be equal to b c 1 (X − 1)(X − 2).   1 a 0 1  ∈ M3×3 (R). Find the set of all Exercise 755 Let A =  a a a a −1 real numbers a for which the minimal and characteristic polynomials of A are equal. Exercise 756 Let F = GF (5). For characteristic polynomial and minimal  a b 4  b b b   3 4 2b   0 0 0 0 0 0

which values of a, b ∈ F are the polynomial of the matrix  2 0 3 3   1 3   0 1  3b 0

equal? What if F = GF (7)? Exercise 757 Let F be a field and let O = A ∈ M3×3 (F ) be a matrix satisfying Ak = O for some positive integer k. Show that A3 = O. Exercise 758 Let F be a field and let A ∈ M3×3 (F ) be a matrix which can be written in the form BC, where B and C are matrices in M3×3 (F ) satisfying B 2 = I = C 2 . Show that A is nonsingular and similar to A−1 . Exercise 759 Let A ∈ M3×3 (Q) be a matrix satisfying the condition that A5 = I. Show that A = I. Exercise 760 Let n be a positive integer and let α be an endomorphism of Mn×n (C), considered as a vector space over C, which satisfies the condition that α(A) is nonsingular if and only if A is nonsingular. Show that α is an automorphism. Exercise 761 Let F be a field and let n be a positive integer. Let (F ) be a matrix having characteristic polynomial p(X) = X n + A∈M n−1 n−1 n×ni k j i=0 ci X . Show that, for each k ≥ n, we have A = j=0 bj (k)A , where (1) bj (n) = −cj for all 0 ≤ j ≤ n − 1; (2) b−1 (k) = 0 for all k ≥ n; (3) bj (k + 1) = bj−1 (k) − aj bn−1 (k) for all k ≥ n and all 0 ≤ j ≤ n − 1.

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Exercise 762 Show that there is! no matrix A ∈ M2×2 (R) satisfying the −1 0 condition that A2 = , where c > 1. 0 −c Exercise 763 Let V be a vector space finitely generated over C and let α ∈ End(V ) be diagonalizable. If W is a nontrival subspace of V invariant under α, is the restriction of α to W necessarily diagonalizable? Exercise 764 Find all rational numbers a satisfying the condition the endomorphism of Q3 represented with respect to some basis by the matrix   1 0 0  1 a 0  is diagonalizable. 0 0 1 Exercise 765 Let n be a positive integer and let B ∈ Mn×n (R) be a matrix all entries of which are positive. Let r > ρ(B). Show that (1) All the matrix A = rI − B is nonsingular; (2) All nondiagonal entries of A are nonpositive; (3) All entries of A−1 are nonnegative; and (4) If a + bi ∈ C is an eigenvalue of A, then a > 0. Exercise 766 Let V be a vector space of finite odd dimension over R and let α1 , . . . αk be distinct mutually-commuting endomorphisms of V, for some k > 1. Show that these endomorphisms have a common eigenvector.     a 2b  b   2a     Exercise 767 Show that the endomorphisms α :   c  →  2d  and d 2c     a c  b   d  4    β :   c  →  a  of Q are diagonalizable and commute. Find a d b basis of Q4 relative to which both α and β are represented by diagonal matrices. Exercise 768 Let A ∈ M3×3 (Q) have characteristic polynomial X 3 − bX 2 + cX − d. For all n ≥ 3, show that An = tn−1 A + tn−2 adj(A) + (tn − btn−1 )I, n−i−2j n−2i−3j i j b cd . where tn = 2i+3j≤n (−1)i i+j j i+j

13 Krylov subspaces

Let V be a vector space over a field F and let α ∈ End(V ). If 0V = v0 ∈ V then the subspace F {v0 , α(v0 ), α2 (v0 ), . . .} of V is called the Krylov1 subspace of V defined by α and v0 . The elements of this subspace are precisely those vectors in V of the form p(α)(v0 ), where p(X) ∈ F [X], and so it is natural to denote it by F [α]v0 . It is clear that F [α]v0 is invariant under α. We claim that dim(F [α]v0 ) = 1 if of and only if v0 is an eigenvector of α. Indeed, if v0 is an eigenvector k α associated with an eigenvalue c then for each p(X) = j=0 aj X j ∈ k k j j F [X] we have p(α)(v0 ) = j=0 aj α (v0 ) = j=0 aj c v0 ∈ F v0 , proving that F [α]v0 = F v0 and so dim(F [α]v0 ) = 1. Conversely, assume that dim(F [α]v0 ) = 1. Then F [α]v0 = F v0 since F v0 is a one-dimensional subspace of F [α]v0 . In particular, α(v0 ) ∈ F v0 and so there exists a scalar c such that α(v0 ) = cv0 , which proves that v0 is an eigenvector

1 Alexei Nikolaevich Krylov was a Russian applied mathematician who, at the end of the 19th century, developed many of the methods mentioned here in connection with the solution of differential equations.

267

268

13. Krylov subspaces

of α. Note that in any case the set {v0 , α(v0 ), α2 (v0 ), . . .} is a generating set for F [α]v0 over F and so dim(F [α]v0 ) can be used to measure how “far” v0 is from being an eigenvector of α. (13.1) Proposition: Let V be a vector space over a field F and let α ∈ End(V ). If 0V = v0 ∈ V then F [α]v0 is the intersection of all subspaces of V containing v0 and invariant under α. Proof: Since F [α]v0 contains v0 and invariant under α, it certainly contains the intersection of all such subspaces of V. Conversely, if W is a subspace of V which contains v0 and invariant under α, then p(α)(v0 ) ∈ W for all p(X) ∈ F [X] and so F [α]v0 ⊆ W. Thus we have the desired equality. As a first example of the use to which we can put Krylov subspaces, we will see how to use the minimal polynomial to solve systems of linear equations. Let V be a vector space over a field F and let V ∞ be the space kof all infinite sequences of elements of V. Every polynomial p(X) = j=0 aj X j ∈ F [X] defines an endomorphism θp of V ∞ by   k k k aj vj , aj vj+1 , aj vj+2 , . . . . θp : [v0 , v1 , . . .] →  j=0

j=0

j=0

Note that if p(X) = c is a polynomial of degree no greater than 0, then θp = σ c . It is also easy to verify that θpq = θp θq = θq θp for all p(X), q(X) ∈ F [X]. A sequence y ∈ V ∞ is linearly recurrent if and only if there exists a polynomial p(X) ∈ F [X] with y ∈ ker(θp ). In this case, we say that p(X) is a characteristic polynomial of y. If p(X) ∈ F [X] is a characteristic polynomial of y ∈ V ∞ and if q(X) ∈ F [X] is a characteristic polynomial of z ∈ V ∞ then θpq (y + z) = θq θp (y) + θp θq (z) = [0, 0. . . .] and so p(X)q(X) is a characteristic polynomial of y + z. It is also clear that p(X) is a characteristic polynomial of cy for all c ∈ F. Thus we see that the set of all linearly recurrent sequences in V ∞ is a subspace of V ∞ , which we will denote by LR(V ). If y ∈ LR(V ), there is precisely one characteristic polynomial which is monic and of minimal degree. This polynomial will be called the minimal polynomial of y. The degree of the minimal polynomial of y will be called the order of recurrence of y. Example: Let F be a field, let n be a positive integer, and let V = Mn×n (F ). If A ∈ V then a polynomial p(X) ∈ F [X] is a characteristic [resp. minimal] polynomial of the sequence [I, A, A2 , . . .] if and only if it was the characteristic [minimal] polynomial of A in the sense of the previous chapter.


269

Example: Let V = F = Q and let y = [a0 , a1 , . . .] ∈ V ∞ be the sequence defined by a0 = 0, a1 = 1, and ai+2 = ai+1 + ai for all i ≥ 0. This sequence is called the Fibonacci sequence. Its minimal polynomial √ is X 2 − X − 1. The roots of this polynomial are 12 (1 ± 5). The number √ 1 5) is called the golden ratio and artists consider rectangles the 2 (1 + sides of which are related by the golden ratio to be of high aesthetic value. This ratio – which appears in ancient Egyptian and Babylonian texts – appears in nature and is basic in the analysis of certain patterns of growth in nature (such as the spirals of a snail shell or a sunflower), of Greek architecture, of Renaissance painting2 , and even such modern designs as the ratio of the dimensions of a credit card or of A4 paper. Notice that ! 1 1 ∈ X 2 − X − 1 is also the characteristic polynomial of the matrix 1 0 √ M2×2 (R), and so the eigenvalues of this matrix are also precisely 12 (1± 5). √ ! 1 √ (1 + 5) and the The eigenspace associated with 12 (1 + 5) is R 2 1 ! √ 1 √ (1 − 5) eigenspace associated with 12 (1 − 5) is R 2 . 1 We note that if V = F and if y ∈ LR(F ) is a sequence having order of recurrence at most n, then there exist algorithms, which are essentially extensions of the euclidean algorithm, to calculate the coefficients of the minimal polynomial of y in an order of n2 arithmetic operations in F. Now let V be a vector space of finite dimension n over a field F and let α be an automorphism of V having minimal polynomial p(X) ∈ F [X]. If w ∈ V then the sequence y = [w, α(w), α2 (w), . . .] belongs to ker(θp ) and hence to LR(V ). Therefore this sequence has a minimal d polynomial q(X) = j=0 cj X j , which divides the polynomial p(X) in F [X]. Since α is an automorphism, we can assume that c0 = 0 and d j−1 (w) then α(u) = w and so so we see that if u = −c−1 0 j=1 cj α

2

Leonardo Fibonacci was born in Italy in the 12th century and educated in Tunis, bringing back the fruits of Arab mathematics to Europe. His book Liber Abaci, written in 1202, contained the first new mathematical research in Christian Europe in over 1000 years. In 1509, Fra Luca Pacioli, one of the most important Renaissance mathematicians, wrote a book, The Divine Proportion, illustrated by his friend Leonardo da Vinci, about the golden ratio.

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u = α−1 (w). In particular, if V = F n for some positive integer n and if α is represented A with respect to the canonical basis, d by a matrix j−1 c A w is the unique solution of the system of then u = −c−1 j 0 j=1 d j−1 then linear equations AX = w. If we set q ∗ (X) = −c−1 0 j=1 cj X ∗ u = q (A)w, and this could be computed quickly were we to already know q(X). How does one calculate q ∗ (X) in practice? One method in use is basically probabilistic: we randomly choose a vector u ∈ F n and compute the minimal polynomial qu (X) of the sequence yu = [u w, u (Aw), u A2 w), . . .] in F ∞ , something which can be done, as we have already observed, in an order of n2 arithmetic operations in F. After that, we check whether the minimal polynomial of yu is also the minimal polynomial of y. In general, it will not be so, but it will divide the minimal polynomial of y and so after a reasonable number of such attempts we will, usually, have enough information on hand to reconstruct the minimal polynomial of y. 

 1 4 4 Example: Let F = GF (5), let A =  4 0 3  ∈ M3×3 (F ), and 1 2 4   3 let w =  1  ∈ F 3 . The sequence w, Aw, A2 w, . . . looks like 2             3 0 4 2 3 0  1 , 3 , 4 , 0 , 0 , 1 ,... . 2 3 3 4 3 0   1 If we choose u =  0  we obtain the sequence yu = [3, 0, 4, 2, 3, 0, . . .] 0 in F ∞

and the minimal polynomial qu (X) of this sequence equals   0 X 2 + 2X + 2. Since qu (A)w =  2  , we see that this polynomial is 3   1 not the minimal polynomial of y. We will try again with u =  2  . 0 For this choice, we get yu = [0, 1, 2, 2, 3, 2, . . .] and this has minimal polynomial X 3 + 3X + 1. Since the minimal polynomial of y has to be a multiple of this polynomial, and has to be of degree 3, it must equal


271



 0 X 3 + 3X + 1 and, indeed, qu (A)w =  0  . Therefore q ∗ (X) = X 2 + 3 0   2 and q ∗ (A)w = qu (A)w =  3  . 1 Now let us return to an important problem which was considered in the previous chapter. Let V be a vector space finitely generated over a field F. Given an endomorphism α ∈ End(V ), how can we find a basis of V relative to which α is represented by a matrix which is as nice as possible? We have already found out when α is diagonalizable. But what if α is not diagonalizable? Given a vector 0V = w ∈ V, there exists a positive integer k such that the set {w, α(w), . . . , αk−1 (w)} is linearly independent but the set {w, α(w), . . . , wk (w)} is linearly dependent. Then {w, α(w), . . . , αk−1 (w)} is a basis for the Krylov subspace F [α]w of V, which is called the canonical basis of this subspace. The restriction of α to F [α]w is represented by a matrix of the form   0 0 . . . 0 c1   1 0 . . . 0 c2     0 1 . . . 0 c3  with respect to the canonical basis, where the    ...    0 ... 1 0 ck−1  0 ... 0 1 ck k scalars c1 , . . . , ck satisfy αk (w) = i=1 ci αi−1 (w). This, of course, is k just the companion matrix of the polynomial X k − i=1 ci X i−1 . Krylov subspaces are also the basis for a family of iterative algorithms, known as Krylov algorithms, used for approximating solutions to systems of equations of the form AX = w, where A ∈ Mn×n (R) or A ∈ Mn×n (C). Similarly, Krylov subspaces are a basis for a family of iterative algorithms, known as Lanczos3 algorithms, used for approximating eigenvalues of sufficiently-nice (e.g. symmetric) matrices. Such algorithms

3

Hungarian-born applied mathematician Cornelius Lanczos developed many important numerical methods for computers in the period after World War II, while working at the US National Bureau of Standards and, later, at the University of Dublin in Ireland.

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work even under the assumption that we don’t even have direct access to the entries of A but do have a “black box” ability to compute Av or AT v for any given vector v ∈ Rn . Of course, they do not work for all matrices, but when they work they tend to be fairly efficient and rapid, and are especially good for large sparse matrices. Moreover, they are also amenable to implementation on parallel computers. Let V be a vector space over a field F. An endomorphism α ∈ End(V ) is nilpotent if and only if there exists a positive integer k satisfying αk = σ 0 . The smallest such integer k, if one exists, is called the index of nilpotence of the endomorphism. Example: Let F be a field and let α be the endomorphism of F 3     a 0 defined by α :  b  →  a  . Then α is a nilpotent endomorphism, c b having index of nilpotence 3. The endomorphism β of F 3 defined by     a −a + 2b + c  is a nilpotent endomorphism, having index 0 β :  b  →  c −a + 2b + c of nilpotence 2. Example: Let F be a field ! and let! α and β be the ! endomorphisms ! a b a 0 2 → and β : → . Both of F defined by α : b 0 b a endomorphisms are nilpotent, but α + β is clearly not nilpotent. If α is a nilpotent endomorphism of a vector space V and w ∈ V ker(α) then the restriction of α to F [α]w is represented with respect to the canonical basis of F [α]w by a matrix of the form   0 0 0 ... 0 0  1 0 0 ... 0 0     0 1 0 ... 0 0   .   ...    0 0 0 ... 0 0  0 0 0 ... 1 0

(13.2) Proposition: Let V be a vector space over a field F and let α be a nilpotent endomorphism of V having index of nilpotence k. Then there exists a vector w ∈ V satisfying the condition that dim(F [α]w) = k.


273

Proof: We know that αk = σ 0 but that there exists a vector 0V = w ∈ V such that αk−1 (w) = 0V . We will have proven the theorem should we are able to show that the set {w, α(w), . . . , αk−1 (w)} is linearly independent. And, indeed, assume that we have scalars a0 , . . . , ak−1 ∈ F k−1 i satisfying index such that i=0 ai α (w) = 0V . Let t be the smallest k−1 k−t−1 i at = 0. Then if we apply the endomorphism α to i=0 ai α (w) we k−1 k 2k−t−2 (w) + at+1 α (w) + . . . + ak−2 α (w) and so at = 0, get 0V = at α which is a contradiction. Therefore we conclude that ai = 0 for all i, and so the set is linearly independent, as required. In particular, we see that if V is a vector space of finite dimension over a field F and if α is a nilpotent endomorphism of V, then the index of nilpotence of α is no greater than dim(V ). (13.3) Proposition: Let V be a vector space finitely generated over a field F and let α be a nilpotent endomorphism of V having index of nilpotence k. If w ∈ V satisfies the condition that dim(F [α]w) = k then the subspace F [α]w of V has a complement in V which is invariant under α.

Proof: We will proceed by induction on k. If k = 1 then α = σ 0 and so F [α]w = F w. Then there is a subset B of V {F w} such that B ∪ {w} is a basis for V, and B is a basis for a complement of F w in V . Thus we can assume that k > 1 and that the result has been established for any vector space finitely generated over F and any nilpotent endomorphism of that space having index of nilpotence less than k. We know that im(α) is invariant under α and that the restriction of α to im(α) is nilpotent, having index of nilpotence k − 1. We know that the set {w, α(w), . . . , αk−1 (w)} forms a basis for F [α]w and so the set {α(w), . . . , αk−1 (w)} forms a basis for the image U of F [α]w under α. Therefore, U = F [α]α(w) is a subspace of im(α) and, by the induction hypothesis, it has a complement W2 in im(α) invariant under α. Let W0 = {v ∈ V | α(v) ∈ W2 }. This is a subspace of V containing W2 , since W2 is invariant under α. But α(v) ∈ W2 ⊆ W0 for all v ∈ W0 and so W0 is also invariant under α. Our first assertion is that V = F [α]w + W0 . And, indeed, if x ∈ V then α(x) ∈ im(α) = U ⊕ W2 and so α(x) = u + w2 , where u ∈ U and w2 ∈ W2 . But u = α(y) for some y ∈ F [α]w and x = y + (x − y). The first summand belongs to F [α]w, whereas, as to the second, we have α(x −y) = α(x)−α(y) = α(x)− u = w2 ∈ W2 and so x −y ∈ W0 , proving the assertion. Our second assertion is that F [α]w∩W0 ⊆ U. Indeed, if x ∈ F [α]w∩W0 then α(x) ∈ U ∩ W2 = {0V } and so x ∈ ker(α). Since x ∈ F [α]w, we

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k−1 know that there exist scalars a0 , . . . , ak−1 such that x = i=0 ai αi (w) k−2 and hence 0V = α(x) = i=0 ai αi+1 (w), which implies that a0 = . . . = ak−2 = 0. Therefore x = ak−1 αk−1 (w) ∈ U, proving the second assertion. In particular, from what we have seen. we deduce that the subspaces W2 and F [α]w ∩ W0 are disjoint. Therefore W2 ⊕ (F [α]w ∩ W0 ) is a subspace of W0 . This subspace has a complement W1 in W0 . Thus we have W0 = W1 ⊕ W2 ⊕ (F [α]w ∩ W0 ) . Our third assertion is that W = W1 ⊕ W2 is a complement of F [α]w in V which is invariant under α, and should we prove this, we will have proven the proposition. Indeed, we immediately note that α(W ) ⊆ α(W0 ) ⊆ W2 ⊆ W and so W is surely invariant under α. Moreover, F [α]w ∩ W = {0V } since this subspace is contained in the intersection of W and F [α]w ∩ W0 , which, by the choice of W, equals {0V }. Finally, V

= F [α]w + W0 = F [α]w + [W1 + W2 + (F [α]w ∩ W0 )] = F [α]w + W1 + W2 = F [α]w + W

and so V = F [α]w ⊕ W.

(13.4) Proposition (Rational Decomposition Theorem): Let V be a vector space of finite dimension n over a field F let α be a nilpotent endomorphism of V having index of nilpotence k. Then there exist natural numbers k = k1 ≥ . . . ≥ kt satisfying k1 + . . . + kt = n, and there exist vectors v1 , . . . , vt in V such that {v1 , α(v1 ), . . . , αk1 −1 (v1 ), v2 , α(v2 ), . . . , αk2 −1 (v2 ), . . . , vt , α(vt ), . . . , αkt −1 (vt )} forms a basis for V. The matrix which represents   A1 O . . . O  O A2 . . . O  , α with respect to this basis is of the form    ... O O . . . At   0 0 ... 0 0  1 0 ... 0 0     where each Ai is of the form   0 1 . . . 0 0  in Mki ×ki (F ).   ... 0 0 ... 1 0 Proof: Choose k1 = k and choose v1 to be any vector not in ker(αk1 −1 ). Then U1 = F [α]v1 has a basis {v1 , α(v1 ), . . . , αk1 −1 (v1 )}. This subspace is invariant under α and of dimension k1 . By Proposition 13.3, we know that we can write V = U1 ⊕ W1 , where W1 is a subspace of V which is also invariant under α. The restriction of α to W1 is a nilpotent endomorphism of W1 having index of nilpotence k2 ≤ k1 . We now return on the above procedure for W1 . We pick an element v2 ∈ W1 ker(αk2 −1 ). Then the subspace U2 = F [α]v2 of W1 has a


275

basis {v2 , α(v2 ), . . . , αk2 −1 (v2 )}. This subspace is invariant under α and of dimension k2 . Moreover, we can write W1 = U2 ⊕ W2 , where W2 is invariant under α. Continuing in this manner, we end up with a decomposition V = U1 ⊕ . . . ⊕ Ut , where each Ui is a subspace of V invariant under α having a basis of the form {vi , α(vi ), . . . , αki −1 (vi )} as above. This proves the first contention of the proposition. The second one follows since Ui = F [α]vi for all i, which leads to a matrix of the desired form. A matrix of the form given in Proposition 13.4 is called a representation of the nilpotent endomorphism α in Jordan4 canonical form. Let V be a vector space over a field F and let α be an endomorphism of V having an eigenvalue c. A vector 0V = v ∈ V is a generalized eigenvector of α associated with c of degree k > 0 if and only if v is in ker((α − cσ 1 )k ) ker((α − cσ 1 )k−1 ). Thus, in particular, the eigenvectors of α associated with c, in the previous sense, are just the generalized eigenvectors of α of degree 1 associated with c. Example: Let α be the endomorphism of R4 represented with respect   2 −2 1 1  0 1 1 1   . This endomorto the canonical basis by the matrix   0 0 2 1  0 0 0 2   2  1   phism has an eigenvector   0  associated with the eigenvalue 1 and an 0   1  0   eigenvector   0  associated with the eigenvalue 2. It also has a gener0   0  −1   alized eigenvector   −1  of degree 2 associated with the eigenvalue 2 0

4 The 19th-century French mathematician Camille Jordan made major contributions to linear algebra, group theory, the theory of finite fields, and the beginnings of topology.

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

 0  −1   and a generalized eigenvector   −1  of degree 3 associated with the −1 eigenvalue 2. We now prove a generalization of Proposition 12.1. (13.5) Proposition: Let V be a vector space over a field F and let α ∈ End(V ) have an eigenvalue c. Then the set of all generalized eigenvectors of α (of all degrees) associated with c, together with 0V , forms a subspace of V. Proof: Let a ∈ F and let v, w ∈ V be generalized eigenvectors of α associated with c, of degrees k and h respectively. Then both v and w belong to ker(α − cσ 1 )h+k and hence the same is true for v + w and av. This means that there exist positive integers s, t ≤ h + k such that v + w ∈ ker((α − cσ 1 )s ) ker((α − cσ 1 )s−1 ) and av ∈ ker((α − cσ 1 )t ) ker((α − cσ 1 )t−1 ), which is what we needed. Let V be a vector space over a field F and let α ∈ End(V ) have an eigenvalue c. The subspace of V defined in Proposition 13.5 is called the generalized eigenspace of α associated with c. (13.6) Proposition: Let V be a vector space over a field F and let α ∈ End(V ) have an eigenvalue c. Let v be a generalized eigenvector of degree k associated with c. Then the set of vectors {v, (α−cσ 1 )(v), . . . , (α−cσ 1 )k−1 (v)} is linearly independent. Proof: Set β = α − cσ 1 and, for each 1 ≤ j ≤ k, let vj = β k−j (v). k Assume that there exist scalars c1 , . . . , ck ∈ F satisfying j=1 cj vj = 0V . k k−1 k−1 k−1 (ck vk ) = ck β (vk ) and so, since Then 0V = β j=1 cj vj = β β k−1 (vk ) = 0V , we conclude that ck = 0. We work backwards in this manner to see that cj = 0 for all 1 ≤ j ≤ k, and so the given set is linearly independent. In particular, let V be a vector space of finite dimension n over a field F and let α ∈ End(V ). If v is a generalized eigenvector of α of degree k associated to an eigenvalue c of α, then we must have k ≤ n. Thus we see that dim(V ) is an upper bound to the degree of generalized eigenvalue of α and we see that the generalized eigenspace of α associated to an eigenvalue c is just ker((α − cσ 1 )n ).


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(13.7) Proposition: Let V be a vector space of finite dimension n over a field F and let α ∈ End(V ) satisfy the condition that the characteristic polynomial p(X) of α is completely reducible, m say p(X) = j=1 (X −cj )nj , where spec(α) = {c1 , . . . cm }. Then there exist subspaces U1 , . . . , Um of V, each of which invariant under α, such that: (1) V = U1 ⊕ . . . ⊕ Um ; (2) dim(Uh ) = nh for each 1 ≤ h ≤ m; (3) For each 1 ≤ h ≤ m, the restriction of α to Uh is of the form ch τ h + β h , where β h ∈ End(Uh ) is nilpotent and τ h is the restriction of σ 1 to Uh . Proof: For each 1 ≤ h ≤ m, consider the endomorphism β h = α−ch σ 1 of V, and let Uh be the generalized eigenspace of α associated with ch . Then Uh is a subspace of V invariant under β h and also invariant under α since for all v ∈ Uh we have β nh α(v) = αβ nh (v) = α(0V ) = 0V . We claim that there exists a positive integer k, independent of h, such that all elements of Uh are generalized eigenvectors of α of degree at most k. Indeed, we see that ker(β h ) ⊆ ker(β 2h ) ⊆ ker(β 3h ) ⊆ . . . and since V is finitely-generated, there are at most a finite number of proper containments. Thus there exists a k such that ker(β kh ) = ker(β k+1 h ) = .... k From here it is clear that ker(β h ) = Uh , proving the claim. In particular, this claim shows that the restriction of β h to Uh is a nilpotent endomorphism having index of nilpotence k. More than that, the restriction of α to Uh equals ch τ h + β h , proving (3). We now notice that if t = h then Ut is invariant under β h . We claim that the restriction of β h to Ut is an automorphism. Since Ut is finitedimensional, it is sufficient to prove that it is a monomorphism. Indeed, suppose that v ∈ Ut ∩ker(β h ). Then there exists a positive integer k such that β kt (v) = 0V and so 0V = β kt (v) = [β h + (ch − ct )]k (v) = (ch − ct )k (v) and, since ch − ct = 0, we must have v = 0V , proving the claim. The next step is to show that the collection {U1 , . . . , Um } of subspaces of V is independent. Indeed, let 1 ≤ h ≤ m and let a subspace of V invariant under β h on Y = Uh ∩ j=h Uj . Then Y is which β h is monic (since Y ⊆ j=h Uj ) and nilpotent (since Y ⊆ Uh ), which is possible only if Y = {0V }. This proves independence, and we will set U = U1 ⊕ . . . ⊕ Um . We want to show that U = V. Let v ∈ U. By the Cayley-Hamilton Theorem (Proposition 12.16) that α annihilates mwe see ni β ] (v) = 0V ∈ U. Supits characteristic polynomial p(X) and so [ i=1 i m pose that β nt 1 (v) ∈ U, say that it is equal to i=1 ui , where uh ∈ Uh for all 1 ≤ h ≤ m. Since β nt 1 is epic when restricted to Uh , for each 1 < h ≤ m, such that h = 1, we can find an elements wh of Uh for each m − h=2 wh ) = u1 ∈ U1 . uh = β nt 1 (wh ) for all such h. Therefore β nt 1 (u m By definition mof U1 , it follows that w1 = u − h=2 wh ∈ U1 . There/ U, then let fore v = h=1 wh ∈ U. If, on the other hand, β nt 1 (v) ∈

278


*t be the +smallest element*of {2, .+. . m} satisfying the condition that t t−1 ni ni (v) ∈ U and (v) ∈ / U. A similar argument to the i=1 β i i=1 β i preceding then shows that we must have v ∈ U. We are left to show that dim(Uh ) = nh for all 1 ≤ h ≤ m. Pick a basis for V which is a union of bases of the Uh . With respect to this basis, the endomorphism α is represented by a matrix of the form   O A1 O . . .  O A2 . . . O   , where each Ah is a matrix representing the re   ... O O . . . Am striction of α to Uh . By Proposition 11.12, mthe characteristic polynomial of α is therefore of the form |XI − A| = h=1 |XI − Ah |. From this decomposition and from the fact that each β h restricts to an automorphism of Ut for all t = h, it follows that the only eigenvalue of the restriction of α to Uh isch , and the algebraic m multiplicity of this eigenvalue is at most m dim(U ) = nh . Since h h=1 h=1 nh , it then follows that dim(Uh ) = nh for each h. Proposition 13.7 shows that when conditions are right – for example when the field F is algebraically closed – and when we are given an endomorphism α of a finite-dimensional vector space, it is possible to choose a basis for V relative to which α is represented in a particularly simple form. We do this in two steps. (I) Write V as a direct sum U1 ⊕ . . . ⊕ Um as above. By choosing a basis for V which is a union of bases of the Uh , we get a matrix representing α composed of blocks strung out along the main diagonal, each representing the restriction of α to one of the subspaces Uh . (II) For each h, we have α = ch τ h + β h , where β h is a nilpotent endomorphism of Uh . We now choose a basis of Uh relative to which β h is represented in Jordan canonical form. Thus, in the end, we have a representation of α by a matrix of the form   O A1 O . . .  O A2 . . . O     , where each block Ah is a matrix with blocks of  ..   . O O . . . Am   ch 0 0 ... 0  1 ch 0 ... 0     0 1 ch . . . 0  the form   on its diagonal (these may be 1 × 1!)   .. ..   . . 0

...

0

1 ch

and all other entries equal to 0. A matrix of this form is called the Jordan canonical form of α. By Proposition 13.7, we see that if V is a vector


279

space finitely generated over a field F and if α is an endomorphism of V having a completely reducible characteristic polynomial in F [X], then there is a basis of V relative to which α can be represented by a matrix in Jordan canonical form. Thus, this can always be done if the field F is algebraically closed. If F is not algebraically closed then it is always possible to extend the field F to a larger field K such that the characteristic polynomial of α is completely reducible in K[X]. Example: Consider the endomorphism α of R4 which  0  0 with respect to the canonical basis by the matrix A =   0 −1

is represented  1 0 0 0 1 0  . 0 0 1  4 −6 4

The characteristic polynomial of this matrix is X 4 −4X 3 +6X 2 −4X +1 = (X − 1)4 and so its only eigenvalue is 1. The matrix A is similar to   1 0 0 0  1 1 0 0   the matrix B =   0 1 1 0  in Jordan canonical form. Indeed, 0 0 1 1   −1 3 −3 1  1 −2 1 0  . B = P AP −1 , where P =   −1 1 0 0  1 0 0 0 Example: Consider the endomorphism α of R5 which is represented   3 0 0 0 0  0 4 2 −1 4    0 0  with respect to the canonical basis by the matrix A =   0 0 2 .  0 1 3 2 1  0 0 0 0 2 The characteristic polynomial of this matrix is (X − 3)3 (X − 2)2 . The ma  2 0 0 0 0  0 3 0 0 0     trix A is similar to the matrix B =   0 1 3 0 0  in Jordan canon 0 0 0 2 0  0 0 0 0 3   0 0 −3 0 −4  0 1 −1 −1 3    −1  3 0 1  ical form. Indeed, B = P AP , where P =  2 1 .  0 0 0 0 −1  −1 0 0 0 0

280


Example: Consider the endomorphism α of C4 which is represented   0 0 2i 0  1 0 0 2i   . The with respect to the canonical basis by A =   −2i 0 0 0  0 −2i 1 0 2 characteristic polynomial of this matrix is (X −2) (X +2)2 . The matrix A   −2 0 0 0  1 −2 0 0   . Indeed, B = P AP −1 , is similar to the matrix B =   0 0 2 0  0 0 1 2   1 0 −i 0  1 0 1 0 −i . where P =   i 0  2 1 0 0 1 0 i We now use Jordan canonical forms to prove a result interesting in its own right. (13.8) Proposition: Let n be a positive integer and let A ∈ Mn×n (C). Then A can be written as a product of two symmetric matrices. Proof: By Proposition 13.7 we know that A is similar to a matrix B in Jordan canonical form. In other words, there exists a nonsingular matrix Q ∈ Mn×n (C) satisfying A = QBQ−1 . If we can write B = CD, where both C and D are symmetric, then A = QBDQ−1 = (QCQT )((QT )−1 DQ−1 ) = (QCQT )((Q−1 )T DQ−1 ), where both QCQT and (Q−1 )T DQ−1 are symmetric. Therefore, without loss of generality, we can assume that A is in Jordan canonical form, say   O A1 O . . .  O A2 . . . O   , where each block Ah is of the form A=   ... O O . . . Am   0 0 ... 0 ah  1 ah 0 ... 0     0  . . . 0 1 a h   ∈ Mnh ×nh (C).   . . .. ..   0 ... 0 1 ah Define the matrix Dh ∈ Mnh ×nh (C) to be [dij ], where

1 if i + j = nh + 1 dij = . 0 otherwise


281

Then Dh is a symmetric matrix satisfying Dh−1 = Dh . Moreover, the   O ... O D1  O D2 . . . O    matrix D =   ∈ Mn×n (C) is also symmetric and ..   . O O . . . Dm satisfies D−1 = D. Furthermore, the matrix  A1 D1 O ... O  D . . . O O A 2 2  C= ..  . O

O

...

    ∈ Mn×n (C) 

Am Dm

is also symmetric and A = CD, as required.

Exercises Exercise 769 Let V = R3 . Find endomorphisms α and β of V satisfying the condition that αβ is not nilpotent but cα + dβ is nilpotent for all c, d ∈ R. Exercise 770 Let V be a vector space over a field F and let α ∈ End(V ) be nilpotent, having index of nilpotence k > 0. Show that σ 1 +α ∈ Aut(V ). Exercise 771 Let V be a vector space finitely-generated over C. Do there exist endomorphisms α and β of V satisfying the condition that σ 1 + αβ − βα is nilpotent? Exercise 772 Let F be a field. Give an example of a nilpotent endomorphism of F 5 having index of nilpotence 3. Exercise 773 Let α be the endomorphism of V = R4 represented with   2 −8 12 −60  2 −5 9 −48   respect to a basis B of V by the matrix   6 −17 29 −152  . 1 −3 5 −26 Show that α is nilpotent and find its index of nilpotence. Exercise 774 Let V be a vector space over a field F and let α ∈ End(V ) be nilpotent. Does βα have to be nilpotent for all β ∈ End(V )? Exercise 775 Let V be a vector space over a field F End(V ) be nilpotent. Find spec(α).

and let α ∈

282


Exercise 776 Let V be a vector space finitely generated over C and let α ∈ End(V ) satisfy spec(α) = {0}. Show that α is nilpotent. Exercise 777 Let V be a vector space over a field F and let α ∈ End(V ) be nilpotent, having index of nilpotence k. Find the minimal polynomial of α. Exercise 778 Let V be a vector space finitely generated over a field F and let α ∈ End(V ) satisfy the condition that for each v ∈ V there exists a positive integer n(v) satisfying αn(v) (v) = 0V . Show that α is nilpotent. Exercise 779 Let F be a field and let α be an endomorphism of F 3   0 a 0 represented with respect to a basis B of F 3 by the matrix  0 0 b  , 0 0 0 where a and b are nonzero scalars. Does there exist a endomorphism β of F 3 satisfying β 2 = α? Exercise 780 Let α be a nilpotent endomorphism of a vector space V over a field F having characteristic 0. Show that there exists an endomorphism β of V belonging to F [α] and satisfying β 2 = σ 1 + α. Exercise 781 Let α ∈ End(R3 ) be represented with respect to the canon    1 2 −2 1 3  . Calculate R[α]  0  . ical basis by the matrix  3 0 1 1 −2 0 Exercise 782 Let V be the space of all infinitely-differentiable functions from R to itself. Let δ be the endomorphism of V which assigns to each function its derivative. What is R[δ] sin(x)? 

   a a+c  b − a  . Find Exercise 783 Define α ∈ End(R3 ) by α :  b  → c b   1 R[α]  1  . 1 Exercise 784 Let V End(V ). Let v ∈ V F [α]v = V.

be a vector space over a field F and let α ∈ be a vector satisfying F [α2 ]v = V. Show that


283

Exercise 785 Given a ∈ R, let αa ∈ End(R4 ) be represented with   0 a 1 0  1 −2 1 1   . For respect to the canonical basis by the matrix   0 0 1 0  0 1 0 −2   0  0    equal to 3? which values of a is the dimension of R[αa ]  0  −1 Exercise 786 Let α ∈ End(R3 )  1 1 ical basis by the matrix  0 1 0 0

be represented with respect to the canon 1 0  . Find the eigenvalues of α and 2

the generalized eigenspace associated with each. Exercise 787 Let V be a vector space over a field F and let α, β ∈ End(V ) satisfy αβ = βα. Let W be the generalized eigenspace of α associated with an eigenvalue a. Show that W is invariant under β. Exercise 788 Let V be a vector space finitely generated over C and let α ∈ End(V ). Show that V is diagonalizable if and only if every generalized eigenvector of α is an eigenvector of α. Exercise 789 Let B = {v1 , v2 , v3 } be the canonical basis of  1 let α be the endomorphism of R3 satisfying ΦBB (α) =  0 0

R3 and  0 2 1 0 . 0 1

Show that W = R{v1 , v3 } and Y = Rv2 are complements of each other in R3 and that each of these spaces is invariant under α.   1 2 0 2 0  ∈ M3×3 (R). Find the Jordan Exercise 790 Let A =  0 2 −2 −1 canonical form of A.   −2 8 6 6  ∈ M3×3 (R). Find the Jordan Exercise 791 Let A =  −4 10 4 −8 −4 canonical form of A.   0 a −b 0 c , Exercise 792 Let O = A ∈ M3×3 (C) be of the form  −a b −c 0 where a, b, and c are real numbers. What is the Jordan canonical form of A?

284


Exercise 793 Let n be a positive integer. If A ∈ Mn×n (C), show that A and AT are similar. Exercise 794 Let A ∈ M5×5 (Q) be a matrix in Jordan canonical form having minimal polynomial (X − 3)2 . What does A look like? Exercise 795 Give an example of a matrix in M4×4 (R) which is not similar to a matrix in Jordan canonical form. Exercise 796 Let V be a vector space finitely generated over a field F and let α and β be nilpotent endomorphisms of V represented with respect to some given basis by matrices A and B respectively. If the matrices A and B are similar, does the index of nilpotence of α have to equal that of β?   a 0 0 Exercise 797 Let F be a field and let A =  1 a 0  ∈ M3×3 (F ). 0 1 a   k a 0 0 ak 0  for all k > 0. kak−1 Show that Ak =  1 k−2 k−1 k k(k − 1)a ka a 2 Exercise 798 Let n be a positive integer and, for all 1 ≤ i, j ≤ n, let pij (X) ∈ C[X]. Let ϕ : C →Mn×n (C) be the function defined by ϕ : z → [pij (z)]. Furthermore, let us assume that ϕ(z) is nonsingular for each z ∈ C. Show that there exists a nonzero complex number d such that |ϕ(z)| = d for all z ∈ C. Exercise 799 For each t ∈ C, let αt be the endomorphism of C3   0 1 0 represented with respect to the canonical basis by the matrix  0 0 0  . t 0 0 Is the representation of αt in  0 Exercise 800 Let A =  0 0

Jordan canonical form dependent on t?  0 4 0 0  ∈ M3×3 (C). Find the set of all 0 0

c ∈ C satisfying the condition that cA is similar to A.

14 The dual space

Let V be a vector space over a field F. A linear transformation from V to F (considered as a vector space over itself) is a linear functional on V. The space Hom(V, F ) of all such linear functionals is called the dual space of V and will be denoted by D(V ). Note that D(V ) is a vector space over F, the identity element of which for addition is the 0-functional, v → 0. Since dim(F ) = 1, we immediately see that every linear functional other than the 0-functional must be an epimorphism1 .

Example: Let F be a field and let n be a positive integer. Any v ∈ F n defines a linear functional in D(F n ) by w → v w.

1

Linear functionals were first studied systematically by the French mathematician Jacques Hadamard, whose long life ranged from the mid 19th century to the mid 20th century. His work on functionals turned them into an important tool in analysis.

285

286

14. The dual space

Example: Let V be a vector space over a field F and let B be a basis for V. Each u ∈ B defines a function fu ∈ F B defined by

1 if u = u fu : u → 0 otherwise and by Proposition 6.2 we know that this function in turn defines a linear functional δ u ∈ D(V ). In particular, if V = F n and if B = {u1 , . . . , un }   a1   is the canonical basis for V, then δ uh :  ...  → ah for each 1 ≤ h ≤ n. an Example: Suppose that V = C(a, b) and that g0 ∈ V. Then the 4b function η : V → R defined by η : f → a f (x)g0 (x)dx belongs to D(V ). Hadamard’s initial work on linear functionals concerned those of 4b the form f → lim a f (x)gn (x)dx for suitable sequences g1 , g2 , . . . in n→∞ V. Example: Let V be the subspace of RR consisting of all infinitelydifferentiable functions f satisfying the condition that there exist real numbers / [a, b]. Then the function 4 ∞ a ≤ b such that f (x) = 0 if x ∈ f → −∞ f (x)dx belongs to D(V ). Elements of D(V ) are known as distributions and play an important role in analysis and theoretical physics. Let F be a field and let n be a positive integer. Then there exists a linear functional tr : Mn×n (F ) → F which assigns nto each matrix the sum of the elements of its diagonal, i.e. tr : [aij ] → i=1 aii . This linear functional is called the trace. This functional will play an important part in our later discussion. Note that v w = tr(v ∧ w) for all v, w ∈ F n . The set of all matrices A ∈ Mn×n (F ) satisfying tr(A) = 0 forms a subalgebra of the general Lie algebra Mn×n (F )− , called the special Lie algebra defined by F n . [bij ] are matrices in Mn×n (F ), then it is If A = [aij ] and B = n n easy to see that tr(AB) = i=1 h=1 aih bhi = tr(BA). We also notice that tr(I) = n, where I is the identity matrix of Mn×n (F ). If the characteristic of the field F does not divide n, we claim that these conditions uniquely characterize the trace. (14.1) Proposition: Let n be a positive integer and let F be a field the characteristic of which does not divide n. Let δ be a linear functional on Mn×n (F ) satisfying the conditions that

14. The dual space

287

δ(AB) = δ(BA) for all A, B ∈ Mn×n (F ) and that δ(I) = n. Then δ = tr. Proof: If {Hij | 1 ≤ i, j ≤ n} is the canonical basis of Mn×n (F ), then it suffices to show that δ(Hij ) = tr(Hij ) for all 1 ≤ i, j ≤ n. In particular, if 1 ≤ i, j ≤ n then δ(Hii ) = δ(Hij Hji ) = δ(H jin Hij ) = δ(Hjj ). n Since I = i=1 Hii , this implies that n = δ(I) = i=1 δ(Hii ) and so δ(Hii ) = 1 = tr(Hii ) for all 1 ≤ i ≤ n. If i = j then H1j Hi1 = O and so δ(Hij ) = δ(Hi1 H1j ) = δ(H1j Hi1 ) = δ(O) = 0 = tr(Hij ) and we are done. By the above, we see that if F is a field, if n is a positive integer, and if A, B ∈ Mn×n (F ), then tr(A • B) = tr(AB) − tr(BA) = 0, where • denotes the Lie product on Mn×n (F ). In fact, the converse of this result is also true – namely that if a matrix C satisfies tr(C) = 0, then C is the Lie product of two other matrices – as has been proven in several more general contexts2 . If n is a positive integer, if F is a field, and if P is a nonsingular matrix in Mn×n (F ), then tr(P AP −1 ) = tr(P P −1 A) = tr(A) and so similar matrices have identical traces. In general, if B and C are fixed matrices in Mn×n (F ) then the functions A → tr(BA) and A → tr(AC) belong to D(Mn×n (F )). The following result shows that traces essentially define all linear functionals on spaces of square matrices. (14.2) Proposition: Let F be a field, let n be a positive integer, and let δ ∈ D(Mn×n (F )). Then there exists a matrix C ∈ Mn×n (F ) satisfying δ : A → tr(AC) for all A ∈ Mn×n (F ). Proof: For each 1 ≤ i, j ≤ n, let Hij be the matrix having (i, j)-entry equal to 1 and all of the other entries equal to 0. Then we know that the set of all such matrices is a basis for Mn×n (F ). Let C = [cij ] ∈ Mn×n (F ) be the matrix defined by cij = δ(Hji ) for all 1 ≤ i, j ≤ n. Then for each n n a H matrix A = [aij ] ∈ Mn×n (F ) we have δ(A) = δ i=1 j=1 ij ij =

2

The first of many proofs of this result was given by Kenjiro Shoda, one of the major figures in 20th-century Japanese algebra.

288

n

14. The dual space

n

i=1

prove.

j=1

aij δ(Hij ) =

n i=1

n j=1

aij cji = tr(AC), as we needed to

(14.3) Proposition: Let F be a field, let n be a positive integer, and let δ ∈ D(Mn×n (F )) be a linear functional satisfying δ(AB) = δ(BA) for all A, B ∈ Mn×n (F ). Then there exists a scalar c ∈ F such that δ(A) = c · tr(A) for all A ∈ Mn×n (F ). Proof: Again, for each 1 ≤ i, j ≤ n, let Hij be the matrix having (i, j)-entry equal to 1 and all of the other entries equal to 0. If 1 ≤ i = j ≤ n then δ(Hij ) = δ(Hii Hij ) = δ(Hij Hii ) = δ(O) = 0. Moreover, for all 1 ≤ j, k ≤ n we have δ(Hjj ) = δ(Hjk Hkj ) = δ(Hkj Hjk ) = δ(Hkk ). Thus we see that there exists a c ∈ F such that δ(Hjj ) = c for all 1 ≤ j ≤ n and from Proposition 14.2 we conclude that δ(A) = tr(A · cI) = c · tr(A) for all A ∈ Mn×n (F ). (14.4) Proposition: Let F be a field, let n be a positive integer, and let A ∈ Mn×n (F ) be a matrix the characteristic polynomial of which is completely reducible. Then tr(A) is the sum of the eigenvalues of A (with the appropriate multiplicities). n i be the characteristic polynomial of Proof: Let p(X) = i=0 ci X A. We know that this polynomial is completely reducible, say p(X) = n n (X −b ), and after multiplying this out, we see that c = − i n−1 i=1 i=1 bi . But from the definition of the characteristic polynomial, we also see that cn−1 = −tr(A). Thus we see that, for any such matrix, tr(A) is the sum of the eigenvalues of A (with the appropriate multiplicities). Example: Let n be a positive integer and let c and d be complex numbers. Can we find all matrices A ∈ Mn×n (C) having the property that c is an eigenvalue of A having geometric multiplicity n−1 and d is an eigenvalue of A having geometric multiplicity 1? (Certainly one such matrix always exists, namely a diagonal matrix with c appearing n − 1 times on the diagonal and d once.) In general, in order for c to be an eigenvalue of A of geometric multiplicity n − 1, the eigenspace connected with it has to be of dimension n − 1. In other words, the nullity of the matrix A − cI must equal n − 1. From this we see that the dimension of the column space of A − cI must equal 1, and so there must exist nonzero     e1 b1     vectors u =  ...  and v =  ...  in Cn such that A − cI = u ∧ v, bn

en

whence A = u ∧ v + cI. Conversely, if A is a matrix of the form u ∧ v + cI, then c is an eigenvalue of A having multiplicity at least n − 1. Note

14. The dual space

289

n that tr(A) = i=1 bi ei + nc. But, as we just noted, tr(A) is also the sum of the eigenvalues of A, counted by multiplicity, and so we want it to equal d + (n − 1)c. Thus we are reduced n to finding vectors u and v as above satisfying the condition that i=1 bi ei = d − c. This is easy to do in concrete cases. Example: Let F be a field, let Ω be a nonempty set, and let V = F Ω . For each a ∈ Ω there exists a linear functional δ a ∈ D(V ) defined by evaluation: δ a : f → f (a). In the case that F is R and Ω is the unit interval of the real line, this functional is known to physicists as the Dirac3 functional. In analysis, evaluation functionals are often used to establish boundary conditions on classes of functions being studied. The following proposition shows that there always enough linear functionals to enable us to distinguish between vectors. (14.5) Proposition: Let V be a vector space of a field F. If v = w are elements of V then there exists a linear functional δ ∈ D(V ) satisfying δ(v) = δ(w). Proof: Since the set {v−w} is linearly independent, it can be completed to a basis B of V. By Proposition 6.2, there exists a linear functional δ ∈ D(V ) satisfying δ(v − w) = 1 and δ(u) = 0 for all u ∈ B {v − w}. This is the linear functional we want. In particular, if 0V = v ∈ V then there is a linear functional δ ∈ D(V ) satisfying δ(v) = 0. We can also extend the idea we used in the proof of Proposition 14.5. Let V be a vector space over a field F and let B be a given basis for V. For each v ∈ B, let δ v ∈ D(V ) satisfy δ v (v) = 1 and δ v (u) = 0 for all v = u ∈ B. We claim that E = { δ v | v ∈ B} is a linearlyindependent subset of D(V ). Indeed, if c1 , . . . , cn are scalars nin F and u1 , . . . , un are elements of B satisfying the condition that i=1 ci δ ui is

3 Paul Dirac, the Nobel-prize-winning 20th-century British physicist, built the first accepted model of quantum mechanics, in which linear functions played a fundamental part.

290

14. The dual space

the 0-functional. Then for all 1 ≤ h ≤ n we have " 0=

n i=1

# ci δ ui

(uh ) =

n

ci δ ui (uh ) = ch .

i=1

This establishes the claim. If V is finitely-generated then Bis finite and so E is a basis for D(V ), since it is easy to check that δ = u∈B δ(u)δ u for all δ ∈ D(V ). Such a basis E for D(V ) is called the dual basis of the basis B for V. If V is not finitely generated, then F E is a subspace of D(V ) composed of all those linear functionals δ ∈ D(V ) satisfying the condition that δ(u) = 0 for at most finitely-many elements u of B. This subspace is called the weak dual space of V. As a consequence of these remarks, we immediately see: (14.6) Proposition: If V is a vector space finitely generated over a field F then dim(V ) = dim(D(V )).

Example: Let a < b be real numbers and let t1 , . . . , tn be distinct real numbers in the closed interval [a, b] of the real line and let W be the subspace of RR consisting of all polynomial functions of degree less than n. Then dim(W ) = n. For each 1 ≤ i ≤ n, let δ i ∈ D(W ) be subset the linear functional defined by δ i : p → p(ti ). We claim that the n if c B = {δ 1 , . . . δ n } of D(W ) is linearly independent. Indeed, i δ i is i=1 n (X −tj ) = the 0-functional and if 1 ≤ h ≤ n, then 0 = ( i=1 ci δ i ) j=h ch (th − tj ), which implies that ch = 0 since the ti are distinct. j=h

Therefore, by Proposition 14.6, B is a basis for D(W ). Since the function 4b p → a p(x)dx also belongs to D(W ), we conclude that there exist real 4b n numbers c1 , . . . , cn satisfying a p(x)dx = i=1 ci p(ti ) for any p ∈ W. Example: Let V be the vector space of all polynomial functions in RR having degree at most 4. Suppose that B = {a1 , . . . , a5 } is a set of distinct positive real numbers and, for each 1 ≤ i4≤ 5, let δ i ∈ D(V ) be a the linear transformation defined by δ i : p(t) −→ 0 i p(t)dt. We claim that B = {δ 1 , . . . , δ 5 } is a basis for D(V ). Indeed, since we know by Proposition 14.6 that dim(D(V )) = 5, all we have to show is that the set B is linearly independent. That is to say, we must show that if there exist real numbers 5 b1 , . . . , b5 satisfying the condition that i=1 bi δ i is the *0-functional, + 5 5 h+1 1 h bi then bi = 0 for all 1 ≤ i ≤ 5. Since b δ (t ) = a i i i=1 i=1 h+1 i for all 0 ≤ h ≤ 4, we must show that the matrix

14. The dual space



a1

 a  2 A=   a5

1 2 2 a1 1 2 2 a2

1 3 3 a1 1 3 3 a2

1 4 4 a1 1 4 4 a2

1 5 5 a1 1 5 5 a2

1 4 4 a5

1 5 5 a5

.. . 1 2 2 a5

1 3 3 a5

291

     

is nonsingular, which we know in fact to be the case since it is just a Vandermonde matrix, which is always nonsingular. Note that Proposition 14.6 is never true for vector spaces which are not finitely generated. The proof of this fact requires a knowledge of the arithmetic of infinite cardinals. Now let V and W be vector spaces over a field F and let α ∈ Hom(V, W ). If δ ∈ D(W ) then δα ∈ D(V ). Moreover, if δ 1 , δ 2 ∈ D(W ) and if v ∈ V then [(δ 1 + δ 2 )α](v) = (δ 1 + δ 2 )α(v) = δ 1 α(v) + δ 2 α(v) = [δ 1 α + δ 2 α](v) and so (δ 1 + δ 2 )α = δ 1 α + δ 2 α. Similarly, if c ∈ F and if δ ∈ D(W ) then c(δα) = (cδ)α. Therefore we see that α defines a linear transformation D(α) ∈ Hom(D(W ), D(V )) by setting D(α) : δ → δα. If V, W, and Y are vector spaces over F and if α ∈ Hom(V, W ) and β ∈ Hom(W, Y ) then it is straightforward to show that D(βα) = D(α)D(β). If α is an isomorphism, then D(α) is also an isomorphism, where D(α)−1 = D(α−1 ). (14.7) Proposition: Let F be a field and let V and W be vector spaces finitely generated over F. Let B = {v1 , . . . , vk } be a basis for V, the dual basis of which is C = {δ 1 , . . . , δ k }, and let D = {w1 , . . . , wn } be a basis for W, the dual basis of which is E = {η 1 , . . . , η n }. If α : V → W is a linear transformation then ΦEC (D(α)) = ΦBD (α). Let ΦBD (α) = [aij ]. For each 1 ≤ i ≤ k we have α(vi ) = Proof: n a w and h=1 (hi h ) so for all 1 ≤ i ≤n k and all 1 ≤ j ≤ n we have D(α)(η j ) (vi ) = η j α(vi ) = h=1 ahi η j (wh ) = aji . But each k δ ∈ D(V ) satisfies δ = i=1 δ(vi )δ i and so, in particular, D(α)(η j ) = ) k k ( i=1 D(α)(η j ) (vi )δ i = i=1 aji δ i , which gives the desired result. We have already seen that, given a vector space V over a field F, we can build the dual space D(V ). Since this too is a vector space over F, we can go on to built its dual space, D2 (V ) = D(D(V )). What do some elements of this space look like? Each v ∈ V defines a function θv : D(V ) → F by setting θv : δ → δ(v). This is indeed a linear function and so is an element of D2 (V ), which we call the evaluation functional at v.

292

14. The dual space

(14.8) Proposition: Let V be a vector space over a field F. The function v → θv is a monomorphism from V to D2 (V ), which is an isomorphism in the case V is finitely generated. Proof: We first have to show that this function is a linear transformation. And, indeed, if v, w ∈ V , if a ∈ F, and if δ ∈ D(V ), then as a direct consequence of the definitions we obtain θv+w (δ) = δ(v + w) = δ(v) + δ(w) = θv (δ) + θw (δ) = [θv + θw ](δ) and so θv+w = θv + θw . Similarly, θav (δ) = δ(av) = aδ(v) = aθv (δ) and so θav = aθv . Thus we have shown that we do indeed have a homomorphism. If v belongs to the kernel of this function then θv (δ) = δ(v) for all δ ∈ D(V ) and so, by Proposition 14.5, we know that v = 0V . Thus it is a monomorphism. Finally, if V is finitely generated then by Proposition 14.6, we see that dim(D2 (V )) = dim(D(V )) = dim(V ) and so any monomorphism from V to D2 (V ) has to be an isomorphism. We should note that the importance of Proposition 14.8 lies not in the existence of an isomorphism between V and D2 (V ), which could be inferred from dimension arguments alone, but in finding a specific, natural, such isomorphism. A proper subspace W of a vector space V over a field F is a maximal subspace if and only if there is no subspace of V properly contained in V and properly containing W. By the Hausdorff Maximum Principle we know that any nontrivial vector space contains a maximal subspace. The maximal subspaces of finitely-generated vector spaces are usually called hyperplanes of the space. We will now use linear functionals in order to characterize these subspaces of V. (14.9) Proposition: A subspace W of a vector space V over a field F is maximal if and only if there exists a linear functional δ ∈ D(V ) which is not the 0-functional, the kernel of which equals W. Proof: Let us assume that W = ker(δ), where δ is a linear functional which is not the 0-functional, and assume that there exists a proper subspace Y of V which properly contains W. Pick y ∈ Y W and x ∈ V Y. These two vectors have to be nonzero and the set {x, y} is linearly independent by Proposition 5.3, since F y ⊆ Y and x ∈ / Y. Set U = F {x, y}. Then ker(δ) and U are disjoint, so the restriction of δ to U is a monomorphism, which is impossible since dim(U ) = 2 and dim(F ) = 1. Therefore W must be a maximal subspace of V. Conversely, let W be a maximal subspace of V and let y ∈ V W. Then F y ∩ W = {0V } and F y + W = V by the maximality of W. Therefore V = F y ⊕ W and so every vector in V can be written in the

14. The dual space

293

form ay + w, where a ∈ F and w ∈ W. The function δ : ay + w → a is a linear functional in D(V ) the kernel of which equals W, as we need. (14.10) Proposition: Let V be a vector space over a field F . , δ n be elements of D(V ). Then δ ∈ F {δ 1 , . . . , δ n } and let δ, δ 1 , . . n if and only if i=1 ker(δ i ) ⊆ ker(δ). Proof: Assume that δ ∈ F {δ 1 , . . . , δ n }. n Then there exist scalars n a1 , . . . , an such that δ = i=1 ai δ i .If v ∈ i=1 ker(δ i ) then δ i (v) = 0 n for all 1 ≤ i ≤ n and so δ(v) = i=1 ai δ i (v) = 0. Thus v ∈ ker(δ). n Conversely, suppose that i=1 ker(δ i ) ⊆ ker(δ). We will proceed by induction on n. First, assume that n = 1. If δ is the 0-functional; then surely we are done. Thus let us assume that this is not the case and let v ∈ V ker(δ). Since ker(δ 1 ) ⊆ ker(δ), this means that δ 1 (v) = 0. Set a = δ 1 (v)−1 δ(v). Then δ(v) = aδ 1 (v) = (aδ 1 )(v) and so v ∈ ker(δ − aδ 1 ). But ker(δ 1 ) ⊆ ker(δ − aδ 1 ) and so this containment is again proper. By Proposition 14.9, ker(δ 1 ) is a maximal subspace of V and so ker(δ − aδ 1 ) = V, which shows that δ = aδ 1 . Now let us assume that we have prove the result for a given n and assume we have linear functionals δ, δ 1 , . . . , δ n+1 in D(V ) satisfying n+1 i=1 ker(δ i ) ⊆ ker(δ). Set W = ker(δ n+1 ) and for each 1 ≤ i ≤ n let β i be the n restriction of δ i to W. Also, let β be the restriction of δ to W. Then i=1 ker(β i ) ⊆ ker(β) and so, by the inductionhypothesis, we know n that there exist scalars n a1 , . . . , an such that β = i=1 ai β i . Therefore the case n = 1, it follows that ker(δ n+1 ) ⊆ ker(δ − i=1 ai δ i ) and, as in n there exists a scalar an+1 such that δ − i=1 ai δ i = an+1 δ n+1 , proving n+1 that δ = i=1 ai δ i . In the context of functional analysis, the following consequence of Proposition 14.9, taken together with the Riesz Representation Theorem (Proposition 16.13), is known as the Fredholm4 alternative, and has many important applications. (14.11) Proposition: Let V and W be vector spaces over a field F, let α ∈ Hom(V, W ), and let w ∈ W. Then w ∈ im(α) if and only if w ∈ ker(δ) for any δ ∈ D(W ) satisfying im(α) ⊆ ker(δ).

4

Swedish mathematician Ivar Fredholm was active in the late 19th century and studied the solvability of integral equations.

294

14. The dual space

Proof: If w ∈ im(α) then the given condition clearly holds. Conversely, assume that w ∈ / im(α) and let B be a basis for im(α). By Proposition 5.3, the set {w} ∪ B is linearly independent and so there exists a subset B of W containing B such that {w} ∪ B is a basis for W. Then F B is a maximal subspace of W and so, by Proposition 14.9, there exists a δ ∈ D(W ) satisfying δ(w) = 0 and im(α) ⊆ F B = ker(δ).

Exercises Exercise 801 Let V = C(0, 1). From calculus we know that each for f ∈ V there exists a maximal element af of {f (t) | 0 ≤ t ≤ 1}. Is the function f → af a linear functional on V ? Exercise 802 Let F = GF (2) and let δ : F 3 → F be the function which   a assigns to each vector v =  b  the value (0 or 1) appearing in the c majority of entries of

v. Is δ a linear functional?

Exercise 803 Let W be a subspace of Q[X] generated by a countablyinfinite linearly-independent set {p1 (X), p Let 2 (X), . . .} of polynomials. ∞ ∞ δ : W → Q be the function defined by δ : i=1 ai pi (X) → i=1 ai deg(pi ) (where only finitely-many of the ai are nonzero). Does δ belong to D(W )? Exercise 804 Find a linear functional δ ∈ D(R3 )    3 functional but which satisfies δ  2  = δ  −1

which is not the 0 3 2  = 0. 1

Exercise 805 Let V = Q[X] and to each vector v = [b1 , b2 , . . .] ∈ Q∞ , let us assign a linear functional δ v ∈ D(V ) defined by δv :

∞ n=1

an X n →

∞

n!an bn+1 .

n=1

Is the function α : Q∞ → D(V ) defined by v → δ v an isomorphism? Exercise 806 Let V be a vector space over a field F and let α, β ∈ D(V ) satisfy the condition that ker(β) ⊆ ker(α). Show that α ∈ F β. Exercise 807 Let F be a field and let 0 = a ∈ F. Let α : F [X] → F be the function defined by α : p(X) → p(a) − p(0). Is α a linear functional?

14. The dual space

Exercise 808 Let V = R3 and consider    a δ 1 :  b  → 2a − b + 3c, δ 2 :  c   a δ 3 :  b  → 4a − 7b + c c

295

the linear functionals  a b  → 3a − 5b + c and c

on V. Is {δ 1 , δ 2 , δ 3 } a basis for D(V )? Exercise 809 Let V be a vector space finitely generated over a field F and let W be a subspace of V having a complement Y in V. Show that D(V ) = W ⊕ Y , where W is a subspace of D(V ) isomorphic to W and Y is a subspace of D(V ) isomorphic to Y. Exercise 810 Let n be a positive integer and let V be the vector space of all polynomial functions from R to itself of degree no more than n. all 0 ≤ k ≤ n, let δ n : V → R be the function defined by δ k : p → 4For 1 k t p(t)dt. Show that {δ 1 , . . . , δ n } is a basis of D(V ). −1       0 0 1   Exercise 811 Let B =  3  ,  1  ,  −1  ⊆ R3 . Find the   −2 −1 3 dual basis of B. Exercise 812 Let n be a positive integer and let V be a vector space of dimension n over a field F. Let B = {δ 1 , . . . , δ n } be a subset of D(V ) and assume that there exists a vector 0V = v ∈ V satisfying δ i (v) = 0 for all 0 ≤ i ≤ n. Show that B is linearly dependent. Exercise 813 Let V be a vector space over a field F. For every subspace W of V, let E(W ) = {δ ∈ D(V ) | ker(δ) ⊇ W }. Show that E(W ) is a subspace of D(V ). Moreover, if W and W are subspaces of V, show that E(W + W ) = E(W ) ∩ E(W ). Exercise 814 Let V be a vector space finitely generated over a field F and let W be a subspace of V. For E(W ) = {δ ∈ D(V ) | ker(δ) ⊇ W }, show that dim(W ) + dim(E(W )) = dim(V ). Exercise 815 Let A, B ∈ M2×2 (R). Show that tr(AB) = tr(A) · tr(B) if and only if |A + B| = |A| + |B|. Exercise 816 Let n be a positive integer and let U be a finite subset of Mn×n (C) which is closed under multiplication of matrices. Show that there exists a matrix A in U satisfying tr(A) ∈ {1, . . . , n} .

296

14. The dual space

Exercise 817 Let n be a positive integer and let F be a field. For any matrix A = [aij ] ∈ Mn×n (F ), define the antitrace of A to be n antitr(A) = i=1 ai,n+1−i . Is the function A → antitr(A) a linear functional on Mn×n (F )? Exercise 818 Let F be a field and let A ∈ M2×2 (F ) be a matrix satisfying tr(A) = tr(A2 ) = 0. Is it necessarily true that A = O? Exercise 819 Let k and n be positive integers. If O = A ∈ Mk×n (R), does there necessarily exist a matrix B ∈ Mn×k (R) satisfying tr(AB) = 0? Exercise 820 Let F be a field and let k = n be positive Let A ∈ Mk×n (F ) and B ∈ Mn×k (F ). Are tr(AB) and necessarily equal?  1 2−i 1+i 0 Exercise 821 Show that the matrices  4 + i 1 + i 1+i 1 1   1 1+i 2−i  3−i 1+i 0  in M3×3 (C) are not similar. 1 27 1−i

integers. tr(BA)  

and

Exercise 822 Let n be a positive integer and let V be the subspace of R[X] composed of all polynomials of degree at most n. What is the dual basis of {1, X, . . . , X n }? Exercise 823 Let V be a vector space over a field F having a maximal subspace W. Show that there exists a linear functional δ ∈ D(V ) satisfying ker(δ) = W. Exercise 824 Let V = R[X]. For all c ∈ R, let εc be the linear functional on V defined by εc : p(X) → p(c). Is {εc | c ∈ R{0, 1}} a linearly-independent subset of D(V )? Exercise 825 Let n be a positive integer. If B and C are elements of Mn×n (R) satisfying tr(B) ≤ tr(C), and if A ∈ Mn×n (R), is it necessarily true that tr(AB) ≤ tr(AC)? Exercise 826 For a matrix A ∈ M3×3 (R), find a positive integer c tr(A) 1 0 1 2 2 . satisfying |A| = tr(A ) tr(A) c tr(A3 ) tr(A2 ) tr(A) Exercise 827 Let k and n be positive integers and let F be a field. Define a function α : Mkn×kn (F ) → Mn×n (F ) as follows: if A ∈ Mkn×kn (F ), write A = [Aij ] , where each Aij is a (k × k)-block. Then set α(A) = [bij ] ∈ Mn×n (F ), where bij = tr(Aij ) for each 1 ≤ i, j ≤ n. Is α a linear transformation? Is it a homomorphism of unital F -algebras?

14. The dual space

297

Exercise 828 Let A be a nonempty set and let V be the collection of all subsets of A, which is a vector space over GF (2). Is the characteristic function of ∅ = D ⊆ A a linear functional on V ? Exercise 829 For each integer n > 1, find a nonsingular matrix A ∈ Mn×n (Q) satisfying tr(A) = 0. Exercise 830 Let n > 1 be an integer and let A ∈ Mn×n (R). Find a symmetric matrix B ∈ Mn×n (R) satisfying tr(A) = tr(B). Exercise 831 Let V be a vector space finitely generated over Q and let α ∈ End(V ) be a projection. Show that there is a basis D of V satisfying the condition that the rank of α equals tr(ΦDD (α)). Exercise 832 Let W be a proper subspace of a vector space V over a field F and let v ∈ V W. Show that there is a linear functional δ ∈ D(V ) satisfying δ(v) = 0 but δ(w) = 0 for all w ∈ W. Exercise 833 Let V be a vector space finitely generated over a field F and let W1 and W2 be proper subspaces of V satisfying V = W1 ⊕ W2 . Show that D(V ) = E1 ⊕ E2 , where Ej = {δ ∈ D(V ) | Wj ⊆ ker(δ)} for j = 1, 2. Exercise 834 Let F be a field and let A ∈ M2×2 (F ). Show that we always have A2 − tr(A)A + |A|I = O. Exercise 835 Let V be the subspace of R∞ consisting of all sequences [a1 , a2 , . . .] ∈ R∞ satisfying the condition that limi→∞ ai exists in R. Define linear functionals δ 1 , δ 2 , . . . , δ ∞ ∈ D(V ) by setting δ h : [a1 , a2 , . . .] → ah for each h = 1, 2, . . . and δ ∞ : [a1 , a2 , . . .] → limi→∞ ai . Is the subset {δ 1 , δ 2 , . . . , δ ∞ } of D(V ) necessarily linearly independent? Exercise 836 Let F be a field and, for each a ∈ F, let εa : F [X] → F be the linear functional defined by εa : p(X) → p(a). Show that the subset {εa | a ∈ F } of D(F [X]) is linearly independent. Exercise 837 Let V be a vector space over a field F and let δ 1 , δ 2 ∈ D(V ) be linear functionals satisfying the condition that δ 1 (v)δ 2 (v) = 0 for all v ∈ V. Show that one of the δ i must be the 0-functional. Exercise 838 Let n > 1 be an integer and let f : Rn → R be a continuous function which maps the 0-vector to 0 and which satisfies the condition that f (v + w) + f (v − w) = 2f (v) for all v, w ∈ Rn . Show that f ∈ D(Rn ). Exercise 839 Let a ∈ R, let n be a positive integer, and let A, B ∈ Mn×n (R). Does there necessarily exist a matrix C ∈ Mn×n (R) satisfying AC + tr(C)A = B?

298

14. The dual space

Exercise 840 Let F be a field and let n be a positive integer. δ: n Let n Mn×n (F ) → F be the linear functional given by δ : [aij ] → i=1 j=1 aij . Find an endomorphism α of Mn×n (F ) satisfying the condition that δ(A) = a · tr(α(A)) for all A ∈ Mn×n (F ). Exercise 841 Let F be a field and let n be a positive integer. Let A, B ∈ Mn×n (F ) be matrices satisfying A2 +B 2 = I and AB +BA = O. Show that tr(A) = tr(B) = 0. Exercise 842 Let F be a field and let n be a positive integer. Given a positive integer k, is it necessarily true that tr(AB)k = tr(Ak )tr(B k ) for all A, B ∈ Mn×n (F )? Exercise 843 Let V be a vector space finitely generated over a field F and let α ∈ End(V ). Show that α and D(α) have identical minimal polynomials. Exercise 844 Let V be a vector space over a field F and let n be a positive integer. Let v1 , . . . , vn be distinct vectors in V and assume that there )exist α ∈ End(V ) and δ ∈ D(V ) such that the matrix ( i−1 δα (vj ) ∈ Mn×n (F ) is nonsingular. Show that the set {v1 , . . . , vn } is linearly independent. Exercise 845 Let W be a subspace of a vector space V over a field F. Show that W is a maximal subspace of V if and only if every complement of W in V has dimension 1. Exercise 846 Let F be a field and let n be a positive integer. For matrices A, B ∈ Mn×n (F ), calculate tr ([AB − BA][AB + BA]) . Exercise 847 Let F be a field and let n be a positive integer. For matrices A, B ∈ Mn×n (F ), do we necessarily have tr((AB)2 ) = tr(A2 B 2 )? Exercise 848 Let n be a positive integer. Can we find matrices A, B ∈ Mn×n (C) satisfying the condition that all eigenvalues of A and of B are positive real numbers, but not all eigenvalues of A + B are positive real numbers? Exercise 849 Let k and n be positive integers, let F be a field, and let O = A ∈ Mk×n (F ). Does there necessarily exist a matrix B ∈ Mn×k (F ) satisfying tr(AB) = 0. Exercise 850 Let V be a vector space of finite dimension n over a , . . . , Wk } of hyperplanes of V field F. A nonempty finite collection {W 15 k Wi = n − k. Is a nonis co-independent if and only if dim i=1

empty subcollection of an co-independent collection of hyperplanes necessarily co-independent?

15 Inner product spaces

In this chapter, we will have to restrict the set of fields over which we work. A subfield F of R is real euclidean if and only if for each 0 ≤ c ∈ F there exists an element d ∈ F satisfying d2 = c and a subfield K of C is euclidean if and only if there exists a real euclidean field F such that K = {a + bi | a, b ∈ F }. It is immediately clear that if K is a euclidean field and c ∈ K, then c ∈ K. Being a euclidean field is intimately tied in with the constructibility of elements of the complex plane by straightedge and compass constructions, and in fact every real euclidean field must contain all those real numbers which are then lengths of line segments obtainable from the unit line segment by straightedge and compass construction methods. Clearly R itself is real euclidean, while Q, as we have already noted, is not; the set real numbers algebraic over Q is real euclidean and properly contained in R. The field C is euclidean, and set of all algebraic numbers is euclidean and properly contained in C. Let V be a vector space over an euclidean field F. A function µ from V × V to F is an inner product on V if and only if: (1) For each w ∈ V, the function v → µ(v, w) from V to F is a linear functional; (2) If v, w ∈ V then µ(v, w) = µ(w, v); (3) If v ∈ V then µ(v, v) is a nonnegative real number, which equals 0 if and only if v = 0V . 299

300

15. Inner product spaces

Note that, in the above situation, if v, w ∈ V then, as a consequence of (2), µ(v, w) + µ(w, v) = 2 Re(µ(v, w)) is also always a real number, though it may of course be negative. In general, once we have fixed an inner product on a space, we will write v, w instead of µ(v, w). A vector space over an euclidean subfield F of C on which we have an inner product defined is called an inner product space. Another term for such spaces, coming from functional analysis, is a pre-Hilbert spaces. Abstract inner product spaces were first studied in an axiomatic manner by Von Neumann. While inner product spaces over general euclidean fields may prove to be interesting in the future, at the moment the study of such spaces is almost universally restricted to spaces over R or C, and so from now on we will do the same and consider only these as possible fields of scalars. When we talk about an inner product space without specifying the field of scalars, we will always assume that it is one of these two fields. Example: Let n be a positive integer and let F be either R or C. We define an inner product on F n , called the dot product, as     a1 b1 n     follows: if v =  ...  and w =  ...  , then we set v · w = ai bi . an

bn

i=1

Note that if F = R, then this product just coincides with the interior product v w which defined earlier. However, that is not true for the case F = C, so we must be very careful to distinguish between the two products. This modification of the definition is necessary since, over C, ! ! ! ! 1 1 1 0 we have = 0, even though = . Hence the i i i 0 interior product is not an inner product as we have defined it in this chapter1 . We can generalize the previous example. If F is either R or C, and if D = [dij ] is a nonsingular matrix in Mn×n (F ), we can define an inner

1 The problem arises because, in C, 0 can be writen as the sum of squares of nonzero elements. A field F in which 0 cannot be the sum of squares of nonzero elements of F is formally real; so R is formally real while C is not. The theory of formally real fields was developed in the 1920’s by the Austrian mathematicians Emil Artin and Otto Schreier.


product on F n by setting     8 a1 b1 9 (  ..   ..   .  ,  .  = a1 an

bn

301



...

an

 b1 )   DDH  ...  , bn

where DH = [dij ]T . The matrix DH is called the conjugate transpose or Hermitian transpose of D, and it again belongs to Mn×n (F ). Conjugate transposes of matrices over C will play an important part in the following discussion; of course, DH = DT for any matrix D ∈ Mn×n (R). The properties of the conjugate transpose are very much like those of the transpose. Indeed, we note that if A, B ∈ Mn×n (C) and c ∈ C, then H (A + B) = AH +B H , (cA)H = cAH , AHH = A, and (AB)H = B H AH . In particular, if A is nonsingular then I = I H = (AA−1 )H = (A−1 )H AH , proving that (A−1 )H = (AH )−1 . Example: If we are given positive real numbers c1 , . . . , cn and consider the diagonal matrix D = [dij ] ∈ Mn×n (R) the diagonal entries of which √ are given by dii = ci for 1 ≤ i ≤ n, then, by the above, we have an inner product on Cn given by  8  

  a1 ..  ,  .   an

 b1 9 n ..  = c a b .  i i i . i=1 bn

Such a product is called a weighted dot product. Weighted dot products are extremely important in statistics and data analysis, where we often want to emphasize the values of certain parameters and de-emphasize others. Example: Let a < b be real numbers and let V = C(a, b). This is, as we have seen, a vector space over R, on which we can define an 4b inner product f, g = a f (x)g(x)dx. Continuity is important here. The set Y of all functions from [a, b] to R which are continuous at all but finitely-many points is a subspace of R[a,b] properly containing C(a, b) 4b but f, g = a f (x)g(x)dx is not an inner product on Y. Indeed, if we select a real number c satisfying a < c < b and define the function f ∈ Y by

1 if x = c f : x → 0 otherwise then f is a nonzero element of Y but f, f = 0. Similarly, if V be the set of all continuous complex-valued functions defined on the closed interval [a, b] in R, then V is a vector space over 4b C, on which we can define an inner product f, g = a f (x)g(x)dx.

302


Example: Let F be R or C, and let V = Mn×n (F ), which is a vector space over F . Define an inner product on V by setting H ) = tr(B H A). If A = [aij ] and B = [bij ], then A, B = tr(AB n n A, B = i=1 j=1 aij bij . those Example: Let V be the subspace of C∞ composed ∞ of all 2 |c | < ∞. sequences [c0 , c1 , . . .] of complex numbers satisfying i=0 i This vector space is very important in analysis, and we can define an inner ∞ product on it by setting [c0 , c1 , . . .], [d0 , d1 , . . .] = i=0 ci di . Let F be R or C, and let W be a subspace of an inner product space V over F. The restriction of this inner product to a function from W ×W to F is an inner product on W. Thus we can always assume that any subspace of an inner product space V inherits the inner-product-space structure of V. Example: Let V be an inner product space over R and let K be the ! a v set of all matrices of the form , where a, b ∈ R and v, w ∈ V. w b Then K is a vector space over R, where addition and scalar multipli! ! ! a + a v + v a v a v = and cation are defined by + w b w + w b + b w! b ! a v ca cv c = . We create the structure of an R-algebra on w b cw cb ! ! a v a v = K by defining an operation • as follows: • w b w b ! aa + v, w av + b v . This algebra is a division algebra, called bb + w, v a w + bw the Cayley algebra, and it is not associative. Indeed, it is the only nonassociative division algebra of finite dimension over R. We now look at some properties of general inner product spaces. (15.1) Proposition: Let V be an inner product space. For v, w1 , w2 ∈ V and for a scalar a, we have: (1) v, w1 + w2 = v, w1 + v, w2 ; (2) v, aw1 = a v, w1 ; (3) 0V , w1 = v, 0V = 0. Proof: From the definition of the inner product, we have v, w1 + w2

= w1 + w2 , v = w1 , v + w2 , v = v, w1 + v, w2 = v, w1 + v, w2 ,


303

which proves (1). We also have v, aw1 = aw1 , v = a w1 , v = aw1 , v = a v, w1 , which proves (2). Finally, 0V , w1 = 00V , w1 = 0 0V , w1 = 0, and similarly v, 0V = 0, proving (3).

By Proposition 15.1, we see that if V is an inner product space over R then for each v ∈ V the function w → v, w from V to F is a linear transformation, but that is not the case for inner product spaces over C.

Let V be a finitely-generatedinner product space, having a basis n n {v1 , . . . , vn }. Given vectors v = i=1 ai vi and w = j=1 bj vj in V, we have 

v, w =

n n i=1 j=1

ai bj vi , vj =

(

a1

...

an

)

 b1   G  ...  , bn

where G = [gij ] is the matrix defined by gij = vi , vj for all 1 ≤ i, j ≤ n. This matrix is known as the Gram2 matrix defined by the given basis.

Example: Let V be the subspace of C[X] consisting of all polynomials of degree at most 5, and let B be the canonical basis for V. Define an 41 inner product on V by setting f, g = 0 f (x)g(x)dx. (Note that we are using the same notation for a polynomial and its corresponding polynomial function in CR .) Then the Gram matrix defined by B is precisely the Hilbert matrix H6 , which we have seen earlier.

2 Jorgen Gram was a Danish mathematician who, at the end of the 19th century, developed computational techniques for inner product spaces in connection with his work for insurance companies.

304


(15.2) Proposition (Cauchy-Schwarz-Bunyakovsky3 Theorem): Let V be an inner product space. If v, w ∈ V, then | v, w |2 ≤ v, v w, w . Proof: If v = 0V or w = 0V then the result is immediate, and so we can assume that both vectors differ from 0V . Let a = − w, v and b = v, v . Then a = − v, w and b = b so 0

≤ av + bw, av + bw = aa v, v + ab v, w + ba w, v + b2 w, w = aab − aba − aba + b2 w, w = b [−aa + b w, w] .

Since v = 0V , it follows that b is a positive real number and so aa ≤ b w, w , which is what we want. Example: If a1 , . . . , an , b1 , . . . , bn , c1 , . . . , cn are real numbers, with ci > 0 for all 1 ≤ i ≤ n, then  :  : n ; n ; n ; ; ci ai bi ≤ < ci a2i  < ci b2i  . i=1

i=1

i=1

Indeed, this is a consequence of the Cauchy-Schwarz-Bunyakovsky Theo    8 a1 b1 9 n  ..   ..  rem, using the weighted dot product  .  ,  .  = i=1 ci ai bi an bn defined on Rn . In general, the Cauchy-Schwarz-Bunyakovsky Theorem is an extremely rich source of inequalities between real-valued functions of several real variables. For example, consider the vectors  √    1 a+b √ 1  a + c  and w =  1  v=√ √ a+b+c 1 b+c

3 Herman Schwarz was a German mathematician who, in the late 19th century, studied spaces of functions and their structure as inner product spaces. Viktor Yakovlevich Bunyakovsky was a Russian student of Cauchy who proved this theorem a generation before Schwarz, but since his work was published in an obscure journal, it was not widely recognized until the 20th century.


305

in R3 , where a, b, and c are positive. Then, by the Cauchy-SchwarzBunyakovsky Theorem, we see that = = = √ a+b a+c b+c + + = v · w ≤ v, v w, w = 6. a+b+c a+b+c a+b+c √ ! 3 √0 ∈ M2×2 (R) is Similarly, we note that the matrix D = 1 2 nonsingular and so, by a previous example, we have an inner product µ on R2 defined by µ

a b

! ,

c d

! =

a b

!T DD

T

c d

! = 3(ac + bd) +

√ 3 (ad + bc).

Applying the Cauchy-Schwarz-Bunyakovsky Theorem, we see that for all real numbers a, b, c, and d we have * ≤

√ +2 3(ac + bd) + 3 (ad + bc) * √ +* √ + 3(a2 + b2 ) + 2 3 ab 3(c2 + d2 ) + 2 3 cd .

In particular, if we take b = d =

√ 3, we see that

(ac + a + c + 3)2 ≤ (a2 + 2a + 3)(c2 + 2c + 3) for all real numbers a and c. Let V be an inner product space. The norm of a vector v ∈ V is defined to be the scalar v = v, v. A vector v satisfying v = 1 is normal. Example: Let V = Rn , and endow V with the dot product. Then > > > a1 > ? > > n > .. > a2i . This norm is known as the euclidean norm on V. > . > = > > i=1 > an > Example: Let4 V = C(−π, π), on which we have defined the inner π product f, g = −π f (x)g(x)dx. For each positive integer k, consider the function fk : x → sin(kx). Then ?6 π √ fk = fk , fk = sin2 (kx)dx = π −π

and so gk =

√1 fk π

is a normal vector in this space.

306


We have seen how the vector space R3 , endowed the cross product ×, is a Lie algebra. It is easy to check that the cross product is related to the dot product on R3 by the relations u × (v × w) = (u · w)v − (u · v)w and (u × v) × w = (u · w)v − (v · w)u for all u, v, w ∈ R3 . Moreover, we have the following identities: (1) v · (v × w) = 0 for all v, w ∈ R3 ; 2 2 2 (2) (Lagrange identity) v × w = v w − (v · w)2 . There are only two possible anticommutative operations on R3 which turn it into an R-algebra satisfying these two identities, namely × and the operation × given by v × w = −(v × w). Furthermore, if n > 3 no such operation can be defined on Rn , except for the case of n = 7. In that case, wecan define an operation × as follows: write elements of R7  v in the form  a  , where v, v ∈ R3 and a ∈ R and then set v      w aw − bv + (v × w) − (v × w ) v  a × b = . −v · w + v · w w v bv − aw + (v × w ) − (v × w) 



     a1 b1 c1 We also note that if u =  a2  , v =  b2  and w =  c2  in a3 b3 c3 a1 b1 c1 3 R then u · (v × w) = a2 b2 c2 . As an immediate consequence, we a3 b3 c3 observe that if u, v, w ∈ R3 then: (1) u · (v × w) = v · (w × u) = w · (u × v); (2) u · (v × w) = 0 if and only if two of these vectors are equal or the set {u, v, w} is linearly dependent. The scalar value u · (v × w) is often called the scalar triple product of the vectors u, v, w, to distinguish it from the vector triple product u × (v × w). (15.3) Proposition: Let V be an inner product space. v, w ∈ V and if a is a scalar, then: (1) av = |a| · v ; (2) v ≥ 0, with equality if and only if v = 0V ;

If


307

(3) (Minkowski’s4 inequality): v + w ≤ v + w ; (4) (Parallelogram law): 2 2 2 2 v + w + v − w = 2 v + w ; (5) (Triangle difference inequality): v − w ≥ |v − w| . Proof: We see that av = av, av = aa v, v = |a|·v , proving (1). Inequality (2) follows immediately from the definition. √ √As for (3), note that if z = a + bi then z + z = 2a ≤ 2|a| = 2 a2 ≤ 2 a2 + b2 = 2|z|. From the Cauchy-Schwarz-Bunyakovsky Theorem, it follows that | v, w | = | w, v | ≤ v · w and so v + w

2

=

v + w, v + w = v, v + v, w + w, v + w, w

≤

v + 2 v · w + w = (v + w)

2

2

2

and that proves (3). Moreover, we know that 2

v + w = v + w, v + w = v, v + v, w + w, v + w, w 2

and v − w = v − w, v − w = v, v − v, w − w, v + w, w . Adding these two gives us (4). Finally, by (3) we have w = w + (v − w) ≤ w + v − w , and so v − w ≥ v − w . Interchanging the roles of v and w and using (1), gives us v − w = w − v ≥ w − v , and so we have (5). 1 v is Note that by Proposition 15.3 we see that if 0V = v ∈ V then v a normal vector. Moreover, if v is normal and c is a scalar satisfying |c| = 1, then cv is again normal.

Example: Let V be an inner product space, and let Ω be a nonempty set. A function f ∈ V Ω is bounded if and only if there exists a real

4 Hermann Minkowski, a German mathematician at the end of the 19th century, built an elegant mathematical framework for the theory of relativity, using four-dimensional noneuclidean geometry.

308


number bf satisfying f (i) ≤ bf for all i ∈ Ω. If f, g ∈ V Ω are bounded functions then, from Minkowski’s inequality, we see that (f + g)(i) ≤ f (i) + g(i) ≤ bf + bg for all i ∈ Ω. If c is a scalar then (cf )(i) = |c| · f (i) ≤ |c|bf for all i ∈ Ω. Thus both f + g and cf are both bounded, and we see that the set of all bounded elements of V Ω is a subspace of V Ω . Example: We now return to a previous example. Let p be an integer greater than 1, not necessarily prime, and let G = Z/(p), on which we have an operation of addition as defined in Chapter 2. Let V = CG , which is a vector space of dimension p over C. On this space, we can define an inner product by setting f, g = n∈G f(n)g(n). Every element n ∈ G defines a function hn : k → cos

2πnk p

+ i sin 2πnk p @ ∈ V as which belongs to V. Given a function f ∈ V, define a function f f@ : n → f, hn = k∈G f (k)hn (−k). This function is called the discrete Fourier transform of f of order p. One can show that the function @ f → f@ is an fact an automorphism of V. Moreover, f (n) = p1 f@(−n) > > > > and f = √1p > f@> for all f ∈ V and all n ∈ G. Example: There are various generalizations of Theorem 15.2 which, as a rule, require more sophisticated methods of complex analysis to prove. For example, the contemporary Greek mathematicians Manolis Magiropoulos and Dimitri Karayannakis have shown that if V is an inner product space and if u, v, and w are distinct elements of V, then 2 |u, v| · |u, w| ≤ u, u [v · w + |v, w|] . In case the set {v, w} is linearly dependent, it is clear that this reduces to the inequality in Proposition 15.2. Inequalities such as these allow us to get better bounds on inner products. For example, let 0 < a < b are real numbers and let V = C(a, b), on which we have the inner product 4b f, g = a f (x)g(x)dx. If u, v, w ∈ V are given by

1 , v : x → sin(x), and w : x → cos(x) x then Proposition 15.2 gives us the bound ? # ?6 "6 6 b b b dx 2 sin (x)dx cos2 (x)dx |u, v| · |u, w| ≤ 2 a x a a u : x →

whereas this result gives us the better upper bound ? 6  "6 # ?6 6 b b b b dx  1  2 2 (x)dx + sin (x)dx cos sin(x) cos(x)dx . 2 a 2 a x a a


309

(15.4) Proposition: Let V be an inner product space and let α ∈ End(V ) satisfy the condition that there exists a real number 0 < c < 1 such that α(v) ≤ c v for all v ∈ V. Then σ 1 + α is monic. Proof: If 0V = v ∈ V then, by Proposition 15.3, v =

v + α(v) − α(v) ≤ v + α(v) + α(v)

= (σ 1 + α)(v) + α(v) and so (σ 1 + α)(v) ≥ v − α(v) ≥ (1 − c) v > 0, which shows that v∈ / ker(σ 1 + α). Thus σ 1 + α is monic. In particular, if V is a finitely-generated inner product space and if α ∈ End(V ) satisfies the condition that there exists a real number 0 < c < 1 such that α(v) ≤ c v for all v ∈ V, then σ 1 + α ∈ Aut(V ). Let β = (σ 1 + α)−1 . If 0V = v ∈ V then v = ≥

(σ 1 + α)β(v) = β(v) + αβ(v) ≥ β(v) − αβ(v) β(v) − c β(v) = (1 − c) β(v) .

Similarly, v ≤ β(v) + αβ(v) ≤ β(v) + c β(v) = (1 + c) β(v) 1 1 and so 1+c v ≤ β(v) ≤ 1−c v for all v ∈ V. Sometimes, however, we need a bit more generality. If V is a vector space over R or C then, in general, a function v → v satisfying conditions (1) - (3) of Proposition 15.3 is called a norm and a vector space on which a fixed norm is defined is called a normed space or, in a functional-analysis context, a pre-Banach space5 . An immediate question is whether every norm defined on a vector space comes from an inner product. The answer is negative: if, for example, we define the > > > a1 > > > n > > norm 1 on Cn by setting > ... > = i=1 |ai |, then this cannot > > > an > 1

5

Normed spaces were first studied at the beginning of the 20th century by the Austrian mathematician Hans Hahn, and then by the American mathematician Norbert Weiner and the Polish mathematician Stefan Banach.

310


come from an inner product since the parallelogram law is not satisfied by this norm. In fact, satisfying the parallelogram law is necessary for a norm to come from an inner product in the following sense: let V be a vector space over R or C on which ψ : V → R ) ( we2 have a 2norm 2 for all v, w ∈ V, − w) = 2 ψ(v) + ψ(w) satisfying ψ(v + w)2 + ψ(v ( ) and write λ(v, w) = 14 ψ(v + w)2 − ψ(v − w)2 . Then it is possible to define an inner product on V relative to which the norm of a vector v is precisely ψ(v). In the case the field of scalars is R, then this inner product is defined by v, w = λ(v, w) and otherwise this inner product is defined by v, w = λ(v, w) + iλ(v, iw). We should point out, however, that for vector spaces V finitely generated over R or C, all norms are equivalent, in the sense that if a and b are norms defined on V then there exist positive real numbers c and d such that c va ≤ vb ≤ d va for all v ∈ V. For vector spaces which are not finitely generated the situation is different, as the following example shows. Example: Let V = C(0, 1), which is a vector space over R, and for each positive integer n, let fn ∈ V be the function defined by

1 − nx if 0 ≤ x ≤ n1 . fn : x → 0 otherwise Let be the norm defined on V by the inner product f, g = 41 f (x)g(x)dx and let ∞ be the norm on V defined by f ∞ = 0 sup { |f (x)| | 0 ≤ x ≤ 1} . Then fn = √13n for all positive integers n, whereas fn ∞ = 1 for all positive integers n. Thus there can be no real number c satisfying f ∞ ≤ c f for all f ∈ V. Example: Let V and W be normed spaces over the same field of scalars F (which is either R or C). If α ∈ Hom(V, W ), set

α = sup

α(v) 0 = v ∈ V V v

where the norm in the numerator is the one defined on W and the norm in the denominator is the one defined on V. We claim that this is a norm defined on Hom(V, W ), called norm induced by the respective norms on V and W. Indeed, as an immediate consequence of the definition we see that α ≥ 0 for all α ∈ Hom(V, W ), with equality happening only when α is the 0-function. We also note that if α is not the 0-function then α is the smallest positive real number c such that α(v) ≤ c v for all v ∈ V.


311

Now let α ∈ Hom(V, W ) and a ∈ F. Then

aα(v) aα = sup 0 = v ∈ V V v

|a|·| α(v) 0 = v ∈ V = |a| · α . = sup V v Finally, if α, β ∈ Hom(V, W ) then

(α + β)(v) 0 = v ∈ V α + β = sup V v

α(v) + β(v) = v ∈ V = sup 0 V v

α(v) + β(v) 0 = v ∈ V ≤ α + β . ≤ sup V v If V = F n and W = F k , endowed with respective dot products and the norms defined by them, then the induced norm on Hom(V, W ) is called the spectral norm. If A ∈ Mk×n (F ), then the spectral norm of A is defined to be the spectral norm of the homomorphism from F n to F k given by v → Av. Example: If p is any positive integer, we can define a norm p on > > > a1 > ? > > n > .. > n |ai |p . For the case p = 2, this of course reduces C by > . > = p > > i=1 > an > p

to the norm coming from the dot product. The proof that this is a norm in the general case relies on a generalization of Minkowski’s inequality: v + wp ≤ vp + wp for all v, w ∈ Cn and any positive integer p. This norm can be used to define a norm on Hom(Cn , Ck ) for positive integers k and n, by setting A B α(v)p αp = sup 0V = v ∈ V vp for any α ∈ Hom(Cn , Ck ). Example: For positive integers k and n, we define the Frobenius norm or Hilbert-Schmidt norm of a matrix A = [aij ] ∈ Mk×n (C) by setting : ; k n 7 ; 2 |aij | = tr(AAH ). A = < F

i=1 j=1

312


Note that this is precisely the norm coming from the inner product on Mk×n (C) given by A, B = tr(AB H ). The norm 1 defined on Cn is important in other contexts as well. Let n be a positive integer and let nθ be the function from Mn×n (C) to R defined by θ : [aij ] → max { i=1 |aij | | 1 ≤ j ≤ n} , which we have already seen when we defined condition numbers. Numerical algorithms that compute the eigenvalues of a matrix, as a rule, make roundoff errors on the order of cθ(A), where c is a constant determined by the precision of the computer on which the algorithm is running. Since the eigenvalues of similar matrices are identical, it is usually useful, given a square matrix A, to find a matrix B similar to A with θ(B) is small. This can often be done by choosing B of the form P AP −1 , where P is a nonsingular diagonal matrix. 

1 0 1 Example: If A =  1 104 102  2 10 0 0 0 if we choose P =  0 1 0 0 10−2

 10−4 10−2  , then θ(A) = 1002. However, 1   , then θ(P AP −1 ) = 3.

Let α be the endomorphism of Cn represented with respect to the canonical basis by a matrix A ∈ Mn×n (C). Then for each v ∈ Cn we have θ(A) v1 ≥ α(v)1 . In particular, if c is an eigenvalue of α associated with an eigenvector v then θ(A) v1 ≥ α(v)1 = |c| · v1 and so θ(A) ≥ |c|. Thus we see that θ(A) ≥ ρ(A), where ρ(A) is the spectral radius of A. This bound is called the Gershgorin bound6 . In fact, we can sharpen this result. (15.5) Proposition (Gershgorin’s Theorem): Let α be the endomorphism of Cn represented with respect to the canonical

6

Semyon Aranovich Gershgorin was a 20th century Russian mathematician. Gershgorin’s theorem was published in a Russian journal in 1931 and was generally ignored, until it was noticed and publicized by the Austrianborn American mathematician Olga Taussky-Todd, one of the most important researchers in the development of numerical linear algebra methods for computers after World War II. Similar results were obtained earlier by Minkowski and Hadamard.


313

basis by the matrix A = [aij ] ∈ Mn×n (C) and, for each 1 ≤ i ≤ n, plane let ri = j=i |aij | . Let Ki be the circle in the complex with radius ri and center aii . Then spec(α) ⊆ K = i=j Ki . 

 b1   Proof: Let c be an eigenvalue of α and let v =  ...  be an bn eigenvector of α associated with c. Let h be an index satisfying|bh | ≥ |bi | = 0 and Av = cv so (c−ahh )bh = j=h ahj bj for all 1 ≤ i ≤ n. Then bh and hence |c − ahh | |bh | ≤ j=i |ahj bj | ≤ |bh | rh . Thus |c − ahh | ≤ rh and so c ∈ Kh ⊆ K, as desired. Example: Let α be the endomorphism of C4 represented with respect   3 1 2 0  4 15 0 −2   . Then to the canonical basis by the matrix A =   −3 0 0 −1  0 0 3 5 spec(A) = {15.32, 4.49, 1.59 ± 2.35i} . These numbers are found in the union K of the following circles in the complex plane: the circle of radius 3 around the point (3, 0); the circle of radius 6 around the point (15, 0), the circle of radius 4 around the point (0, 0), and the circle of radius 3 around the point (5, 0). We furthermore note that spec(A) = spec(AT ) and so, by the same argument, we see that the eigenvalues of α lie in the union K of the following circles in the complex plane: the circle of radius 7 around the point (3, 0), the circle of radius 1 around the point (15, 0), the circle of radius 5 around the point (0, 0), and the circle of radius 3 around the point (5, 0). These circles and the location of the eigenvalues can be seen in the following pictures.

Thus, the eigenvalues of α lie in K ∩ K .

314


Since any polynomial in C[X] is the characteristic polynomial of a matrix, we can use Gershgorin’s Theorem to get a bound on the location of the zeros of any polynomial. However, there are more sophisticated methods available to get much better bounds. There are several generalizations of Gershgorin’s Theorem, the bestknown of which is the following. (15.6) Proposition (Brauer’s Theorem): Let α be the endomorphism of Cn represented with respect to the canonical basis by the matrix A = [aij ] ∈ Mn×n (C) and, for each 1 ≤ i ≤ n, let ri = j=i |aij | . For each 1 ≤ i = j ≤ n, let Kij be the Cassini oval7 {z ∈ C | |z − aii | |z − ajj | ≤ ri rj } in the complex plane. Then spec(α) ⊆ K = i=j Kij . 

 b1   Proof: Let c be an eigenvalue of α and let v =  ...  be an bn eigenvector of α associated with c. Let h and k be indices such that |bh | ≥ |bk | ≥ |bi | for all i = h, k. We know that bh = 0, and we can c, in which assume, as well, that bk = 0 for otherwise we would have ahh = case surely c ∈ K. Since Av = cv, we have (c − ahh )bh = j=h ahj bj and so |c − ahh | |bh | = ahj bj ≤ |ahj | |bj | ≤ |ahj | |bk | = rh |bk | . j=h j=h j=h −1

In other words, |c − ahh | ≤ rh |bk | |bh | . In the same manner, we obtain −1 and so, multiplying these two results together, we |c − akk | ≤ rk |bh | |bk | see that |c − ahh | |c − akk | ≤ rh rk , so c ∈ Khk ⊆ K, as desired. Note that Gershgorin’s Theorem involves n circles, whereas Brauer’s Theorem involves n2 = 12 n(n − 1) ovals.

7

Twentieth-century German mathematician Alfred Brauer emigrated to the United States in 1939; his research was primarily in matrix theory. Giovanni Domenico Cassini was a 17th-century Italian mathematician and astronomer.


315

Example: It is sometimes useful to consider norms on vector spaces V not over subfields of C, namely functions v → v from V to R satisfying conditions (1) - (3) of Proposition 15.3. For example, let F be a finite field and let V = F n for some positive integer n. Define v to be the number of nonzero entries in v, for each v ∈ V. This function is called the Hamming8 norm and is of extreme importance in algebraic coding theory, where one is interested in vector spaces over F in which every nonzero vector has a large Hamming norm. In an example at the beginning of Chapter 3, we showed a vector space of dimension 3 over GF (2), every nonzero element of which has Hamming norm equal to 4. If v and w are vectors in space V over which we have a norm defined, then the distance between v and w is defined as d(v, w) = v − w. When V = Rn on which we have the dot product, this just gives us the ordinary notion of euclidean distance. The ability to define the notion of distance in such spaces is important, since it allows us to measure the degree of error in algorithmic computations by measuring the distance between a computed value and the value predicted by theory. It also allows us to define the notion of convergence. The following proposition shows that this abstract notion of distance indeed has the geometric properties that one would expect from a notion of distance. Example: Let A be a finite set, and let V be the collection of all subsets of A, which is a vector space over F = GF (2). We have a norm defined on V by letting B be the number of elements in B. Then the distance between subsets B and C of A is B + C , namely the number of elements in their symmetric difference. (15.7) Proposition: Let V be a normed space and let v, w, y ∈ V. Then: (1) d(v, w) = d(w, v); (2) d(v, w) ≥ 0, where equality exists if and only if v = w; (3) (Triangle inequality) d(v, w) ≤ d(v, y) + d(y, w). Proof: This is an immediate consequence of Proposition 15.3.

8 Richard Hamming, a 20th-century American mathematician and computer scientist, is best known for his development of the theory of error-detecting and error-correcting codes.

316


Let n be a positive integer. If A = [aij ] *∈ M+n×n (C), and if k > 0 is k (k) 1 h to be I + h=1 h! A . an integer, let us define the matrix P (k) = pij We claim that, for each fixed 1 ≤ i, j ≤ n, the limit

(h)

lim pij

h→∞

exists in

C. Indeed, if B = [bij ] ∈ Mn×n (F ), set m(B) = max1≤i,j≤n |bij |. Then every entry in the matrix A2 equals the sum of n products of pairs of entries of A and so, in absolute value, is equal to at most m(A)2 n. Thus we see that m(A2 ) ≤ m(A)2 n. Similarly, m(A3 ) ≤ m(A2 )m(A)n ≤ m(A)3 n2 and so forth. Thus, in general, nk−1 1 1 k k A m(A)k ≤ [m(A)n] ≤ m k! k! k! and so, in particular, m(P (k)) ≤

k

1 k for all k=0 k! m(A) 1 h r converges h=0 h!

∞

k ≥ 1. But from

absolutely to er calculus we know that the series for each real number r. Therefore the limit we seek exists, and, ! at least (h) by analogy, we are justified in denoting the matrix lim pij by eA . h→∞

(15.8) Proposition: If n is a positive integer A = [aij ] ∈ Mn×n (F ) is a diagonal matrix, where F is R or C, then eA = [bij ] is a diagonal matrix, where

a e ii if i = j bij = . 0 otherwise Proof: This is an immediate consequence of the definition.

In particular, this implies that if B ∈ Mn×n (F ) is similar to a diagonal matrix then B and eB have the same eigenvectors, while the eigenvalues of eB are the exponentials of the eigenvalues of B. 

A1 O  O A2  Actually, we can do a bit better: if A =   O O  A e 1 O  O eA2  each Ah is a square matrix, then eA =   O O

... ... .. . ... ... ... .. . ...

 O O    , where  Am  O O   .  Am e

Example: If O = A ∈ Mn×n (F ), where F is either R or C, is a matrix for which there exists a positive integer t such that At = O,


such integer, then eA  1 2 0 −1  , we have 0 0  1 1 eA = I + A + A2 =  0 2 0

and if k is the least  0 example, if A =  0 0

0 0

Example: If A = B=

0 −r

r 0

!

k 0

B

then e = 

1 Example: If A =  1 1   eA = 

1 1 1

=I+

k

1 h h=1 h! A .

Thus, for

 3 1 2 1 −1  . 0 1

! ∈ M2×2 (R), then eA = cos(r) − sin(r)

317

sin(r) cos(r)

!

1 0

k 1

! ; if

.

 1 1  ∈ M3×3 (R), then 1 1 3 1 3e − 3 1 3 2 3 + 3e 1 3 1 3e − 3

2 1 3 3 + 3e 1 1 3 3e − 3 1 3 1 3e − 3

1 1 3 3e − 3 1 3 1 3e − 3 2 1 3 3 + 3e

  .

If P ∈ Mn×n (F ) is nonsingular, where F is R or C, then k k 1 h 1 −1 −1 A P =I+ (P AP )h I+ P h! h! h=1

h=1

−1

for each k and so P −1 eA P = eP AP . Thus we see that the exponentials of similar matrices are themselves similar. This is very important in calculations. In particular, if A is diagonalizable there exists a nonsingular matrix P such that P −1 AP is a diagonal matrix D = [dij ] and so P −1 eA P = eD is also a diagonal matrix. Thus eA is diagonalizable whenever A is. If (A, B) is a commuting pair of matrices in Mn×n (F ), then as a direct consequence of the definition we see that eA eB = eA+B = eB eA . But this is not true in general, as the following example shows. Example: If A = 1 1 0 1

!

e−1 0

0 1

! =

0 1 0 0 e−1 0

! and B = 1 1

! =

e−1 0

−1 0

0 0

1 − e−1 1

! , then eA eB = ! = eA+B .

318


This fact is significant when it comes to calculating eA in many cases. For example, suppose that A is an n × n matrix having a single eigenvalue c of multiplicity n. Then for each scalar t, the matrices ctI and ∞ k k t(A − cI) commute and so etA = etcI et(A−cI) = (etc I) k=0 tk! (A − cI) k and, from the Cayley-Hamilton Theorem, we know that (A − cI) = O n−1 k k for all k ≥ n. Thus we see that etA = (etc I) k=0 tk! (A − cI) and so there exists a polynomial p(X) ∈ F [X] satisfying etA = p(A). We also note that if A is nonsingular then A and A−1 commute so eA e−A = eA−A = eO = I, proving that eA is nonsingular and e−A = (eA )−1 . A similar proof can be usedto show that if A has distinct eigenvalues {c1 , . . . , cn } and if pk (X) = j=k (ck − cj )−1 (X − cj I) for all 1 ≤ k ≤ n n then for any scalar t we have etA = k=1 etck pk (A). We have thus seen that eA makes sense for any square matrix A over the real or complex numbers. Indeed, matrix exponentials play an important role in solutions of systems of linear differential equations. What about, say, cos(A) and sin(A)? We know that the cosine function has a Maclauren representation cos(x) =

∞ (−1)i i=0

(2i)!

x2i .

For each natural number n, let us consider the polynomial pn (X) =

n (−1)i i=0

(2i)!

X 2i .

Then we can surely calculate pn (A) for each n and see whether sequence of such matrices converges in some sense. However, there is other possibility. We know that for any real or complex number z have cos(z) = 12 [eiz + e−iz ] and so we can just define cos(A) to be matrix 12 [eiA + e−iA ], which we know always exists. 

the anwe the

 cos(1) 0 0  and 0 cos(1) 0 Example: We see that cos(I) =  0 0 cos(1)    2 + 1 cos(3) 1 cos(3) − 1 1 cos(3) − 1  1 1 1 3 3 3 3 3 3   cos  1 1 1  =  31 cos(3) − 13 23 + 13 cos(3) 13 cos(3) − 13  . 1 1 2 1 1 1 1 1 1 3 cos(3) − 3 3 cos(3) − 3 3 + 3 cos(3)


Similarly, we know that sin(z) = iA − e−iA ]. sin(A) to be −i 2 [e

−i iz 2 [e

319

− e−iz ] and so we can define

Exercises Exercise 851 Let V = C(−1, 1) and let a > − 12 be a real number. Is the )a−1/2 41 ( f (t)g(t)dt function µ : V × V → R defined by f, g = −1 1 − t2 an inner product on V ? Exercise 852 Is the function µ : R2 × R2 → R defined by ! ! a1 b1 µ: , → a1 (b1 + b2 ) + a2 (b1 + 2b2 ) a2 b2 an inner product on R2 ? Exercise 853 Is the function µ : R2 × R2 → R defined by ! ! a1 b1 µ: , → a1 b1 − a1 b2 − a2 b1 + 4a2 b2 a2 b2 an inner product on R2 ? Exercise 854 Is the function µ : R3 × R3 → R defined by     a1 b1 µ :  a2  ,  b2  → a1 b1 + 2a2 b2 + 3a3 b3 + a1 b2 + a2 b1 a3 b3 an inner product on R3 ? Exercise 855 Verify whether the function µ : R[X] × R[X] → R defined by µ : (f, g) → deg(f g) is an inner product on R[X]? Exercise 856 Give an example of a function µ : R2 × R2 → R which satisfies the first two conditions of an inner product, which does not satisfy ! ! 1 1 the third, but does satisfy µ , = 1. 0 0 Exercise 857 Is the function µ : R[X] × R[X] → R defined by   ∞ ∞ ∞ ∞ 1 i j  ai bj → ai X , bj X µ: i + j +1 i=0 j=0 i=0 j=0 an inner product on R[X]?

320


Exercise 858 Let V be the vector space of all continuous functions from R to itself. Let µ : V × V → R be the function given by µ : (f, g) → 4t lim 1t −t f (s)g(s)ds. Is µ an inner product? t→∞

 c1   Exercise 859 Let n be a positive integer and let v =  ...  ∈ Rn . Is cn 

the function µv : R[X1 , . . . , Xn ] × R[X1 , . . . , Xn ] → R defined by µv : (p, q) → p(c1 , . . . , cn )q(c1 , . . . , cn ) an inner product on R[X1 , . . . , Xn ]? Exercise 860 Let a < b be real numbers and let V = C(a, b). Let h0 ∈ V be a function satisfying the condition that h0 (t) > 0 for all a < t < b. Show that the function µ : V × V → R defined by µ : (f, g) → 4b f (x)g(x)h0 (x)dx is an inner product on V. a Exercise 861 Let c and d be given realnumbers. Find ! !a necessary b1 a1 , → ca1 b1 + and sufficient condition that the function µ : a2 b2 da2 b2 be an inner product on R2 . Exercise 862 Is the function µ : R3 × R3 → R defined by     b1 a1 µ :  a2  ,  b2  → a21 b2 + b21 a2 + (a3 b3 )2 a3 b3 an inner product on R3 ? Exercise 863 Let V be an inner product space over R and let n > 1 be an integer. For positive real numbers a1 , . . . , an , define the function     v1 w1 n     µ : V n × V n → R by µ :  ...  ,  ...  → i=1 ai vi , wi . Is µ vn

wn

an inner product on V n ? Exercise 864 Let n be a positive integer and let V be the subspace of R[X] consisting of all polynomials of degree n. Is the function most n at µ : V × V → R defined by µ : (p, q) → i=0 p ni q ni an inner product on V ? Exercise 865  a1  .. by µ :  . an

Let 0 < n ∈ Z. Is the function µ : Cn × Cn → C defined    b1 n   ..   ,  .  → i=1 ai bn−i+1 an inner product? bn


321

Exercise 866 Let {u, v} be a linearly-dependent subset of an inner prod2 uct space V, not containing 0V . Show that u v = v, u u. Exercise 867 Let V = C2 on which we have defined the dot product, and let !D = {v ∈ V | v = 1} . Find {Av, v | v ∈ D} , where A = 1 0 ∈ M2×2 (C). 0 0 Exercise 868 Let n be a positive integer and let {v1 , . . . , vk } be a set of vectors in Rn satisfying vi · vj ≤ 0 for all 1 ≤ i < j ≤ k. Show that k ≤ 2n and give an example in which equality holds. Exercise 869 Let n be a positive integer and let A ∈ Mn×n (C) satisfy 2 A2 = A. Is it necessarily true that AH = AH ? Exercise 870 Let V be an inner product space and let v = v be vectors in V. Show that there exists a vector w ∈ V satisfying v, w = v , w . Exercise 871 Let V be an inner product space finitely generated over its field of scalars, and let B = {v1 , . . . , vn } be a basis of V. Show that there exists a basis {w1 , . . . , wn } of V satisfying the condition that

1 if i = j vi , wj = . 0 otherwise Exercise 872 Let W be a subspace of a vector space V over R and let Y be a complement of W in V. Define an inner product µ on W and an inner product ν on Y. Is the function from V × V → R defined by (w + y, w + y ) → µ(w, w ) + ν(y, y ) an inner product on V ? Exercise 873 Let V = C(0, 1). Let A = {f1 , . . . , fn } be a linearlyindependent subset of V and define a function u : R × R → R by n u : (a, b) → j=1 fj (a) cosj (b). Show that if h ∈ V and if there exists a 41 function g ∈ V such that h(x) = 0 u(x, y)g(y)dy for all x ∈ R, then h ∈ RA. Exercise 874 Let V be an inner product space over R. For each real number a, set U (a) = {v ∈ V | v, v ≤ a}. Given a real number a, find a real number b such that v + w, v + w ∈ U (b) for all v, w ∈ U (a). Exercise 875 Let V be an inner product space and let α ∈ End(V ). 2 Show that α(v), v v, α(v) ≤ α(v) for every normal vector v ∈ V. Exercise 876 For real numbers a1 , . . . , an , show that  :  : ; n ; n n ; ; 2/3 4/3 ai ≤ < |ai |  < |ai |  . i=1

i=1

i=1

322


Exercise 877 (Binet-Cauchy identity) For u, v, w, y ∈ R3 , show that (v × w)(y × u) = (v · y)(w · u) − (v · u)(y · w). Exercise 878 Let v be a normal vector in R3 . Show that the function αv : R3 → R3 defined by αv : w → v × (v × w) + w is a projection in End(R3 ). Exercise 879 For u, v, w, y ∈ R3 , show that u·w u·y (u × v) · (w × y) = v·w v·y

.

Exercise 880 For nonnegative real numbers a, b, and c, show that √ (a + b + c) 2 ≤ a2 + b2 + b2 + c2 + a2 + c2 . Exercise 881 For real numbers 0 < a ≤ b ≤ c, show that √ b2 + c2 ≤ 2 a ≤ (b − a)2 + (c − a)2 . Exercise 882 Let n be a positive integer and let A ∈ Mn×n (R) be a matrix the n Gershgorin circles of which are mutually disjoint. Prove that all of the eigenvalues of A are real. +2 4 *4 1 1 Exercise 883 Show that 0 f (x)dx ≤ 0 f (x)2 dx for any f ∈ C(0, 1). Exercise 884 Let f : R →R be the constant function x → 1. Calculate f when f is considered as an element of C(0, π2 ) and compare it to f , when f is considered as an element of C(0, π). Exercise 885 Let V be an inner product space over R and let v, w ∈ V satisfy v + w = v + w . Show that av + bw = a v + b w for all 0 ≤ a, b ∈ R. Exercise 886 Let V be an inner product space over R. Show that 2 2 u, v = 14 u + v − 14 u − v for all u, v ∈ V. Exercise 887 Let V = C(0, 1) on which we have defined the inner prod41 uct f, g = 0 f (t)g(t)dt. Let W be the subspace of V generated by the function x → x2 . Find all elements of W normal with respect to this inner product. Exercise 888 Let V be an inner product space over R and assume that v, w ∈ V are nonzero vectors satisfying the condition v, w = v · w . Show that Rv = Rw. Exercise 889 Let V be an vector space over R on which we have two inner products, µ and µ defined, which in turn define distance functions d and d respectively. If d = d , does it necessarily follow that µ = µ ?


323

Exercise 890 (Apollonius’ identity9 ) Let V be an inner product > >2 2 2 2 space. Show that u − w + v − w = 12 u − v + 2 > 12 (u + v) − w> for all u, v, w ∈ V. Exercise 891 Let V be an inner product space over R and let θ : V × V × V → R be the function defined by 2

2

2

2

θ(v, w, y) = v + w + y + v + w + y − v − w − y − v − w + y . Show that, for any v, w, y ∈ V, the value of θ(v, w, y) does not depend on y. Exercise 892 Let V be an inner product space over R and let n > 2.   v1 n   vi . Show Let θ : V n → V be the function defined by θ :  ...  → n1 >  > > n  > that >vi − θ  i=1 > >

> >2 > > v1 > > n > 2 .. > = v − n > >   i . > > i=1 > > vn

vn

i=1

>2 v1 > > .. > . >  . > vn >

Exercise 893 Let V be an inner product space over R and let v and 2 w be nonzero vectors in V. Show that |v, w| = v, v w, w if and only if the set {v, w} is linearly dependent. Exercise 894 Let n be a positive integer and let be a norm defined on Cn . For each A ∈ Mn×n (C), let A be the spectral norm of A. If A ∈ Mn×n (C) is nonsingular, show that every singular matrix >−1 > B ∈ Mn×n (C) satisfies A − B ≥ >A−1 > . Does there necessarily exist a singular matrix B for which equality holds? Exercise 895 Let V be a vector space over R and let be a norm defined on V. Show that |v − w| ≤ v − w for all v, w ∈ V. Exercise 896 Let V be an inner product space finitely generated over R and let δ ∈ D(V ). Pick v0 ∈ V. Show that for each real number e > 0

9 Greek geometer Apollonius of Perga, who worked in Alexandria in the third century BC, in his famous book Conics, was the first to introduce the terms “hyperbola”, “parabola”, and “ellipse”.

324


there exists a real number d > 0 such that |δ(v) − δ(v0 )| < e whenever v − v0 < d. Exercise 897 Let V be an inner product space. For any u, v, w ∈ V, 0 1 1 1 2 2 1 d(u, w) 0 d(u, v) show that ≤ 0. 2 0 d(v, w)2 1 d(u, v) 2 1 d(u, w) d(v, w)2 0 Exercise 898 Let n > 1 be an integer. Show that there is no norm v → v defined on Cn satisfying

Av n 0V = v ∈ C AF = sup v for all A ∈ Mn×n (C). Exercise 899 Let n > 1 be an integer. For each A ∈ Mn×n (C), let A = ρ(A), the spectral radius of A. Does this turn Mn×n (C) into a normed space? Exercise 900 Let p > 2 be prime and let n be a positive integer. For each 1 ≤ i ≤ n, define w(i) = min{i − 1, p − i + 1}. Does the function   a1 n   w(i)ai turn GF (p)n into a GF (p)n → R defined by  ...  → an

i=1

normed space? Exercise 901 Let 0 < p < 1  a1  f :  ... an

and let f : Rn → R be defined by  #1/p " n  p |ai | → i=1

is not a norm but does satisfy the inequality f (v + w) ≤ 2(1−p)/p [f (v) + f (w)] for all v, w ∈ Rn . Exercise 902 Let n > 1 and let A ∈ Mn×n (C). Show that there are infinitely-many other matrices in Mn×n (C) having the same Gershgorin circles as A. Exercise 903 Let A = [aij ] ∈ M2×2 (C) and let K be the Cassini oval defined by A. Show that every point on the boundary of K is an eigenvalue of a matrix B ∈ M2×2 (C) defining the same Cassini oval.

16 Orthogonality

Let V be an inner product space and let 0V = v, w ∈ V. From Proposition 15.2 we see that v, w + w, v ≤1 −1 ≤ 2 v · w and so there exists a real number 0 ≤ t ≤ π satisfying cos(t) =

v, w + w, v . 2 v · w

This number t is the angle between v and w. Note that if we are working over R, then v, w . cos(t) = v · w Example: If V = Rn is endowed with the dot product, and if 0V = v, w ∈ V then, using analytic geometry, it is easy to show that the angle as defined here is indeed the angle between the straight line determined by v and the origin, and the straight line determined by w and the origin. If we define different inner products on V, we build in this manner various non-euclidean geometries in n-space. Example: Let V = C(0, 1), on which we have defined the inner product 41 f, g = 0 f (x)g(x)dx. In particular, consider the functions f : x → 5x2 325

326

16. Orthogonality

√ √ 5 7 and g = 3, and the angle t √ 41 1 between f and g satisfies cos(t) = 15 (5x2 )(3x)dx = 14 15. 0 and g : x → 3x. Then f =

Vectors v and w in an inner product space V are orthogonal if and only if v, w = 0. In this case we write v ⊥ w. We note that if 2 2 2 2 2 v ⊥ w then v + w = v + v, w + w, v + w = v + w . A nonempty subset D of V is a set of mutually orthogonal vectors if v ⊥ w whenever v = w in D. Example: We have already seen that if v, w ∈ R3 , then v ·(v ×w) = 0. This says that a vector v is orthogonal to v × w, for any vector w. The same is also true for w and v × w and so we see that if {v, w} is a linearly-independent subset of R3 then the set {v, w, v × w} is linearly independent and so is a basis of R3 . Moreover, as an immediate consequence of the Lagrange identity on R3 ,     0 0 we see that if v × w =  0  and v · w = 0 then either v =  0  or 0 0   0 w =  0  . If v, w ∈ R3 , then the angle t between them satisfies the 0 condition that v · w = (v · w) cos(t). Using the Lagrange identity, we see that ) 2 2 2 2 2( v × w = v w − (v · w)2 = v w 1 − cos2 (t) 2

2

= v w sin2 (t) and so v × w = (v · w) | sin(t)|. Thus | cos(t)| =

v × w . v · w

Example: If V = C2 on which we have the dot product, then it is ! ! 2 + 3i 1+i easy to see that ⊥ . −1 + 5i −i Example: Let V = C(−1, 1), on which we have defined the inner 41 product f, g = −1 f (x)g(x)dx. For all i ≥ 0, define the functions pi ∈ V as follows: p0 : x → 1; p1 : x → x; and 2h + 1 h xph (x) − ph−1 (x) whenever h > 1. ph+1 : x → h+1 h+1 These polynomial functions are known as Legendre polynomials. It is easy to verify that pi ⊥ ph whenever i = h.

16. Orthogonality

327

On the same space, we can define another inner product, namely 6 f, g =

1

−1

f (x)g(x) √ dx. 1 − x2

For each i ≥ 0, define the function qi ∈ V by setting q0 : x → 1; q1 : x → x; and qh+1 : x → 2xqh (x) − qh−1 (x) whenever h > 1. These polynomial functions are known as Chebyshev1 polynomials. It is again easy to verify that qi ⊥ qh whenever i = h. Both of the these products are special instances of a more general construction. For any −1 < r, s ∈ R,4 it is possible to define an inner product 1 on C(−1, 1) by setting f, g = −1 f (x)g(x)(1 − x)r (1 + x)s dx. The set of polynomial functions which are mutually orthogonal with respect to this inner product is called the set of Jacobi polynomials of type (r, s). Such polynomials are important in many areas of numerical analysis, and in particular in numerical integration. (16.1) Proposition: Let field of scalars F . (1) If v ∈ V satisfies v (2) If ∅ = A ⊆ V and v ⊥ w for all w ∈ A, then

V

be an inner product space over a

⊥ w for all w ∈ V, then v = 0V . if v ∈ V satisfies the condition that v ⊥ w for w ∈ F A.

Proof: (1) is an immediate consequence of the fact that if v = 0V then v, v = 0. Now assume that ∅ = A ⊆ V and that v ⊥ w for all w ∈ A. If y ∈ F A then there n ∈ A and scalars n exist elements w1 , . . . , w n a1 , . . . , an such that y = i=1 ai wi and so v, y = i=1 ai v, wi = 0, whence v ⊥ y. (16.2) Proposition: Let V be an inner product space and let A be a nonempty set of nonzero mutually-orthogonal vectors in V. Then A is linearly independent.

1 Adrien-Marie Legendre was one of the firstrate mathematicians who worked in France during the time of the revolution and the generation after it. Among other things, he served on the committee that defined the metric system. Pafnuty Lvovich Chebyshev, a 19th-century Russian mathematician, made important contributions to both pure and applied mathematics.

328

16. Orthogonality

Proof: Let {v1 , . . . , vn } be a finite n subset of A and assume that there such that exist scalars c1 , . . . , cn i = 0V . Then, for 1 ≤ h ≤ n, i=1 ci v n n c v , v = we have ch vh , vh = i i h i=1 i=1 ci vi , vh = 0V , vh = 0 and hence ch = 0. Thus any finite subset of A is linearly independent, and therefore A is linearly independent. If V is an inner product space then any vector 0V = w ∈ V defines a function v, w w π w : v → w, w from V to itself, which is in fact a projection the image of which is the subspace of V generated by {w}. This easily-checked remark is the basis for the following theorem. (16.3) Proposition (Gram-Schmidt Theorem): Any finitelygenerated inner product space V has a basis composed of mutually-orthogonal vectors. Proof: We will proceed by induction on dim(V ). If dim(V ) = 1 the result is immediate. Therefore we can assume that the proposition is true for any inner product space of dimension k, and assume that dim(V ) = k + 1. Let W be a subspace of V of dimension k. By the induction hypothesis, there exists a basis {v1 , . . . , vk } of W composed of mutuallyk orthogonal vectors. Let v ∈ V W and set vk+1 = v − i=1 π vi (v). This vector does not belong to W since v ∈ / W. Therefore {v1 , . . . , vk+1 } is a generating set for V. Moreover, for 1 ≤ j ≤ k, we have vk+1 , vj = v, vj −

k v, vj v, vi vi , vj = v, vj − vj , vj = 0 vi , vi vj , vj i=1

and so vk+1 ⊥ vj for all 1 ≤ j ≤ k. By Proposition 5.3, it follows that the set {v1 , . . . , vk+1 } is linearly independent and so is a basis for V. We should note that the proof of Proposition 16.3 is an algorithm, called the Gram-Schmidt process, which is easy to implement by a computer program to create a basis composed of mutually-orthogonal vectors of V, when we are given a basis of any sort for the space. 

  3 0  0   1   Example: Let v1 =   0  , v2 =  2 0 1

   , and v3 



 3  −1   =   3  2

be vectors in R4 , on which we have defined the dot product. The set

16. Orthogonality

329

{v1 , v2 , v3 } is linearly independent and so generates a three-dimensional subspace W of R4 . Let us use the Gram-Schmidt process to build a basis for W composed of mutually-orthogonal vectors. Indeed, we define   0  1   u1 = v1 , u2 = v2 − π u1 (v2 ) =   2  , and u3 = v3 − π u1 (v3 ) − π u2 (v3 ) = 1   0   1  −13  then {u1 , u2 , u3 } is a basis for W, the vectors of which are 6  4  5 mutually orthogonal. Example: Let V = C(−1, 1), on which we have defined the inner 41 product f, g = −1 f (x)g(x)dx. For all i ≥ 0, let fi be the polynomial function fi : x → xi . Then for each n > 0, the set {f0 , . . . , fn } is linearly independent and so forms a basis for a subspace W of V. We now apply the Gram-Schmidt process to this basis, to obtain a basis {p0 , . . . , pn } of vectors in V which are mutually orthogonal, where the pj are precisely the Legendre polynomials we introduced earlier. Actually, the assumption that we have a basis in hand when initiating the Gram-Schmidt process is one of convenience rather than necessity. We could begin with an arbitrary generating set {v1 , . . . , vn } for the given space. In that case, at the hth stage of the process we would begin by checking whether vh is a linear combination of the set of mutually-orthogonal vectors {u1 , . . . , uh−1 } we have already created. If it is, we just discard it and go on to vh+1 . We should point out that the Gram-Schmidt process is not considered computationally stable – small errors and roundoffs in the computational process accumulate rapidly and can lead at the end to a significant difference between the true solution and the computed solution. There are, fortunately, other more sophisticated methods of constructing a basis composed of mutually-orthogonal vectors from a given basis. (16.4) Proposition (Hadamard inequality): Let n be a positive integer, let A = [aij ] ∈√Mn×n (R) be a nonsingular matrix, and let e = |A|. Then |e| ≤ g n nn , where g = max{|aij | | 1 ≤ i, j ≤ n}. Proof: Denote the rows of A by v1 , . . . , vn . Then {v1 , . . . , vn } is a basis for V = Rn and so, using the Gram-Schmidt method, we can find a new basis {u1 , . . . , un } for V , on which we consider the dot product, composed of mutually-orthogonal vectors, and defined by setting h−1 u1 = v1 and uh = vh − j=1 chj uj , where chj = (vh · uj )(uj · uj )−1 .

330

16. Orthogonality

If B ∈ Mn×n (R) is the matrix the rows of which  1 0 0 ...  c21 1 0 ... A = CB, where C =   ... cn1 cn2 . . . cn,n−1

are u1 , . . . , un , then  0 0   . Since C is a  1

lower-triangular matrix, its determinant is the product of the entries on its diagonal, namely 1. Therefore e = |B|. By looking at the Gram-Schmidt method, we see that ui ≤ vi for all 1 ≤ i ≤ n. Moreover, since the ui are mutually orthogonal, we see that 2 matrix defined by dii = ui BB T = D, where D = [dij ] is the diagonal n 2 for all 1 ≤ i ≤ n. Therefore (e)2 = BB T | = |D| = √ i=1 ui . Now let g = max{|aij | | 1√≤ i, j ≤ n}. Then ui ≤ vi ≤ g n for all 1 ≤ i ≤ n and so |e| ≤ g n nn , as desired. Let V be an inner product space having a subspace W. Let W ⊥ = {v ∈ V | v, w = 0 for all w ∈ W } . By Proposition 16.1, we know that W ⊥ is a subspace of V. Since v, v = 0 for all 0V = v ∈ V, it is clear that W and W ⊥ are disjoint. Also, again by Proposition 16.1, we see that V ⊥ = {0V } and {0V }⊥ = V. The space W ⊥ is called the orthogonal complement of W in V, and this name is justified by the following result: (16.5) Proposition: Let W be a subspace of a finitely-generated ⊥ inner product space V. Then V = W ⊕ W ⊥ and W = W ⊥ . Proof: By Proposition 16.3, we know that it is possible to find a basis {v1 , . . . , vk } of W which is composed of mutually-orthogonal vectors, and by the construction method used in the proof of this proposition, we see that this can be extended to a basis {v1 , . . . , vn } of V, the elements of which are still mutually orthogonal. Thus vi ∈ W ⊥ for all k < i ≤ n, proving that V = W + W ⊥ . But we already know that W and W ⊥ are disjoint and so we have W ⊕ W ⊥ . Moreover, {vk+1 , . . . , vn } is a basis ⊥ for W ⊥ and so W = W ⊥ . In particular, if V is an inner product space having a subspace W then we have a natural projection of W ⊕ W ⊥ onto W, called the orthogonal projection. The image of a vector v ∈ W ⊕ W ⊥ under this projection is the unique element of W closest to v, according to the distance function defined by the inner product on V, in the sense of the following theorem. (16.6) Proposition: Let W be a subspace of an inner product space V and let v = w + y, where w ∈ W and y ∈ W ⊥ . Then v − w ≥ v − w for all w ∈ W, with equality holding if and only if w = w.

16. Orthogonality

331

Proof: If w ∈ W then v − w

2

= w − w + y = w − w + y, w − w + y = w − w , w − w + y, w − w + w − w , y + y, y = w − w , w − w + y, y 2

=

w − w + y = w − w + v − w 2

2

and from here the result follows immediately.

2

2

One of the important problems in computational algebra is the following: given an endomorphism α of a finitely-generated inner product space and a vector 0V = v0 ∈ V, find an efficient procedure to define an orthogonal projection onto the Krylov subspace F [α]v0 . One of the first of these is the Arnoldi process, a modification of the Gram-Schmidt process. Several variants of this procedure have been devised, depending on special properties of α. This process is not considered as computationally efficient as the Lanczos algorithm mentioned earlier. Arnoldi’s process is also the basis for the GMRES algorithm (GMRES = generalized minimal residual) for solution of systems of linear equations, devised by Yousef Saad and Martin Schultz in 1986. Note that Proposition 16.5 is not necessarily true if the space V is not finitely generated, as the following example shows. Example: Let V = R(∞) . For each h ≥ 0, let vh be the sequence in which the hth entry equals 1 and all other entries equal 0. Then B = {vh | h ≥ 0} is a basis for V composed of mutually-orthogonal vectors. Let W = R{v0 − v1 , v1 − v2 , . . .}. This subspace of V is proper ⊥ then there exists a nonnegative since v0 ∈ V W. If 0 V = y ∈ W n integer n such that y = i=0 ai vi . where the ai are real numbers and an = 0. But then an = y, vn − vn+1 = 0, and that is a contradiction. Therefore we have shown that W ⊥ = {0V }, despite the fact that W = V. Moreover, in this case V = W ⊕ W ⊥ and (W ⊥ )⊥ = V = W. Let V be an inner product space. A nonempty subset A of V is orthonormal if and only if the elements of A are mutually orthogonal, and each of them is normal. Thus, for example, the canonical basis of Rn , equipped with the dot product, is orthonormal. Example: Let V =4 C(−π, π), on which we have an inner product π defined by f, g = π1 −π f (x)g(x)dx. Then We have an orthonormal 0 1 subset √12 ∪ {sin(nx) | n ≥ 1} ∪ {cos(nx) | n ≥ 1} of V . R Example: 4 ∞Let V 2be the subspace of R consisting of all functions f for which −∞ |f (x)| dx is finite, where the norm is taken with respect

332

16. Orthogonality

4∞ to the inner product f, g = −∞ f (x)g(x)dx defined on V. Let h ∈ V be the function defined by   1 for 0 < x ≤ 12 −1 for 12 < x ≤ 1 . h : x →  0 otherwise This function is known as the Haar2 wavelet. For each j, k ∈ N define j j j/2 j the 0 function h1k ∈ V by setting hk : x → 2 h(2 x − k). Then the subset hjk | j, k ∈ N of V is orthonormal. Haar wavelets have important applications in image compression.

V

(16.7) Proposition: Every finitely-generated inner product space has an orthonormal basis.

Proof: By Proposition 16.3, we know that V has a basis {v1 , . . . , vn } the elements of which are mutually orthogonal. For each 1 ≤ i ≤ n, let −1 wi = vi vi . Then each wi is normal and {w1 , . . . , wn } is a basis for V, the elements of which remain mutually orthogonal. We can modify the Gram-Schmidt method to provide an algorithm for constructing an orthonormal basis from any given basis of a finitely-generated inner product space V, by normalizing each basis element as it is created. This has the added advantage of tending to reduce accumulated roundoff and truncation errors. The examples after Proposition 16.3 and Proposition 16.6 show that inner product spaces which are not finitely generated may have orthonormal bases as well, but this is not always true. Making use of the Hausdorff Maximum Principle, it is possible to show that every inner product space V has a maximal orthonormal set, which must be linearly independent by Proposition 16.2. Such a subset is called a Hilbert subset of V. Clearly, a subset A of V is a Hilbert subset if and only if for every 0V = y ∈ V there exists a v ∈ A satisfying v, y = 0. If V is finitely generated then any Hilbert subset of V is a basis for V, but this is not necessarily true for inner product spaces which are not finitely generated.

2

The twentieth-century Hungarian mathematician Alfr´ ed Haar worked primarily in analysis.

16. Orthogonality

333

Example: It is of course possible that a finitely-generated inner product space may have many different orthonormal bases. For example, the canonical basis of R4 is orthonormal, as is the basis      0 0   1 1 −1   0   √   √   ,  12  ,  12  0   √   √   2 2  0 0 0

 0     0  ,  .   0    1  

(16.8) Proposition: Let V be a finitely-generated inner product basis {v1 , . . . , vn }. If x = n space having anorthonormal n a v and y = b v are vectors in V, then x, y = i i i i i=1 i=1 n a b . i i i=1 Proof: By the properties of the inner product, we have x, y = C D n n n n n = i=1 ai vi , j=1 bj vj i=1 j=1 ai bj vi , vj = i=1 ai bi , as desired. (16.9) Proposition: Let V be a finitely-generated inner product space having anorthonormal basis {v1 , . . . , vn }. Then each n v ∈ V satisfies v = i=1 v, vi vi . n Proof: We know that v = i=1 ai vi ,for some scalarsa1 , . . . , an . Then n n for each 1 ≤ h ≤ n we have v, vh = i=1 ai vi , vh = i=1 ai vi , vh = ah vh , vh = ah , which yields the desired result. The coefficients v, vi encountered in Proposition 16.9 are called the Fourier coefficients of the vector v with respect to the given orthonormal basis.

Example: Consider the vector space C(−1, 1) over R, on which 41 we have the inner product f, g = −1 f (x)g(x)dx. We want to find a polynomial function of degree at most 3 which most closely approximates the function f : x → sin(x) on the interval [−1, 1]. To do so, consider the subspace V of C(−1, 1) generated by the functions pi : x → xi for 0 ≤ i ≤ 3 and f. Apply the Gram-Schmidt process to the getan orthonormal basis {p0 , . . . , p3 , f } of V to {q0 , . . . , q3 , g}, 7 7basis 1 3 5 3 2 1 where q0 : x → 2 ; q1 : x → 2 x; q2 : x → 2 2 x − 2 ; and 7 7 5 3 9 q3 : x → 2 2 x − 6 x . By Proposition 16.6 and Proposition 16.9, we know that the polynomial function of degree at most 3 which most

334

16. Orthogonality

closely approximates the function f is coefficients f, qi are given by 6

f, q0

=

f, q1

=

f, q2

=

f, q3

= =

3 i=0

f, qi qi , where the Fourier

1

1 sin(x)dx = 0; −1 2 6 1 "= # √ 3 sin(x)x dx = 6 (sin(1) − cos(1)) = 0.738; 2 −1 6 1 "= # 3 2 1 5 x − sin(x)dx = 0; 2 2 2 −1 6 1 "= # 5 3 9 7 x − x sin(x)dx 2 2 6 −1 √ √ (14 14) cos(1) − (9 14) sin(1) = −0.034;

Thus the polynomial function we seek is given by u : x → −0.315x3 + 0.998x. The following diagram shows the graphs sin(x) and u(x) over a slightly larger interval, in which u(x) is represented by the dashed line and sin(x) by the solid line.

(16.10) Proposition: Let F be R or C and let k and n be positive integers. Let A ∈ Mk×n (F ) be a matrix the columns of which are linearly independent in F k . Then there exist matrices Q ∈ Mk×n (F ) and R ∈ Mn×n (F ) such that (1) A = QR; (2) The columns of Q are orthonormal with respect to the dot product on F k ; (3) R is nonsingular and upper-triangular.

16. Orthogonality

335

Proof: Let u1 , . . . , un be the columns of A. Apply the Gram-Schmidt process to the set {u1 , . . . , un } and then normalize each of the resulting vectors to obtain an orthonormal set {v1 , . . . , vn } of vectors in F k . Let Q ∈ Mk×n (F ) be the matrix having n columns v1 , . . . , vn . Then, by Proposition 16.9, we see that ui = j=1 (ui · vj )vj for all 1 ≤ i ≤ n, and so A = QR, where R = [rij ] ∈ Mn×n (F ) is given by rij = uj · vi for all 1 ≤ i, j ≤ n. This matrix is clearly nonsingular. Moreover, we note that the Gram-Schmidt process is such that vj is orthogonal to u1 , . . . , uj−1 for all 2 ≤ j ≤ n and so rij = 0 when i > j. Therefore R is also upper-triangular. A decomposition of a matrix in the form given by Proposition 16.10 is called a QR-decomposition. Such decompositions form a basis of many important numerical algorithms, and are widely used, for example, in computing eigenvalues of large matrices. The use is primarily iterative. If A is an n × n matrix over R or C the eigenvalues of which have distinct absolute values and if we can indefinitely perform the iteration (1) A1 = A; (2) If Ai has a QR-decomposition Ai = Qi Ri then set Ai+1 = Ri Qi ; then, under rather mild conditions on A, the sequence A1 , A2 , . . . of matrices tends to an upper triangular matrix in which the eigenvalues of A appear in decreasing order of absolute value along the diagonal.3 One of the major advantages of QR-decompositions is that they are easy to update. If we are given a decomposition A = QR, and then the matrix A is altered slightly to obtain a matrix A by changing a few of its entries, it is relatively easy to alter Q and R to get a QR-decomposition for A . This is important since many applications of linear algebra involve solving successive systems of linear equations of the form A(i) X = w(i) , where A(i+1) and w(i+1) are obtained from A(i) and w(i) by relatively minor modifications, based on data from some external source which is periodically updated. The following algorithm is used to compute a QR-decomposition of a matrix A ∈ Mk×n (F ) with columns u1 , . . . , un :

3

QR-decompositions were developed independently by Swiss computer scientist Heinz Rutishauser, one of the fathers of ALGOL, by Russian computer scientist Vera Kublanovskaya, and by J. G. F. Francis of the British computer manufacturer Ferranti Ltd.

336

For (1) (2) (3)

16. Orthogonality

i = 1 to n do steps (1) - (3): v i = ui ; For j = 1 to i − 1 set rji = ui · vj and vi = vi − rji vj ; −1 vi . Set rii = vi and vi = rii

Then Q is the matrix with columns v1 , . . . , vn and R = [rij ]. Note that step (3) presupposes that we have already checked that the set of columns of A is linearly independent. If not, then we have to add an initial check to insure that rii is nonzero, before we attempt to invert it. As already noted, the Gram-Schmidt method is not numerically stable and hence neither is this algorithm for finding a QR-decomposition. It can be modified to produce a somewhat more stable algorithm by replacing the definition of rji in step (2) by rji = vi · vj . (16.11) Proposition: Let V be a finitely-generated inner product space having an orthonormal basis {v1 , . . . , vn }. Then for all v, w ∈ V : n (1) (Parseval’s identity) v, w = i=1 vi , v vi , w ; n 2 2 (2) (Bessel’s identity4 ) v = i=1 |vi , v| . Proof: Parseval’s identity follows from the calculation 8 n 9 n n v, w = v, vi vi , w = v, vi vi , w = vi , v vi , w i=1

i=1

i=1

and Bessel’s identity derives from this in the special case v = w.

The following results shows that orthogonality can be used to determine the relation between two different inner products defined on a vector space over R. (16.12) Proposition: Let V be a vector space over R on which we have defined two inner products, µ1 and µ2 . For i = 1, 2, let

4 Wilhelm Bessel was a 19th century astronomer and friend of Gauss; his mathematical work came as a result of his research on planetary orbits. Little is known about the life of Marc-Antoine Parseval, a French mathematician who published only five short papers at the end of the 18th century, and no picture of him survives.

16. Orthogonality

337

Yi = {(v, w) ∈ V × V | µi (v, w) = 0}. Then the following conditions are equivalent: (1) There exists a positive real number c such that µ2 = c2 µ1 ; (2) Y1 = Y2 ; (3) Y1 ⊆ Y2 . Proof: Since it is clear that (1) implies (2), and (2) implies (3), all we have to prove is that (3) implies (1). Therefore, assume (3). First let us consider the case dim(V ) = 1, i.e. the case in which V = R. Then, for i = 1, 2, the scalar bi = µi (1, 1) is nonzero. Set d = µ2 (1, 1)/µ1 (1, 1). If a, b ∈ R, then √ µ2 (a, b) = abµ2 (1, 1) = abdµ1 (1, 1) = dµ1 (a, b) and so, taking c = d, we have established (1). Thus we can assume that dim(V ) ≥ 2. For each i = 1, 2, and each v ∈ V, let vi = µi (v, v) > 0. Without loss of generality, we can assume that there exist elements v, w ∈ V and positive real numbers a < b such that v2 = a v1 and w2 = b w1 , since otherwise we would immediately have (1). Suppose that w = dv for some 0 = d ∈ R. Then w2 = |d| · v2 = |d|a · v1 a w1 and so a = b, which is contrary to our assumption that a < b. Therefore we conclude that the set {v, w} is linearly independent. Normalizing v and w with respect to µ1 if necessary, we can furthermore assume that v1 = 1 = w1 . We claim that (v, w) ∈ / Y1 . Indeed, assume otherwise. Then 2

2

µ1 (v + w, v − w) = µ1 (v, v) − µ1 (w, w) = v1 − w1 = 0 and so (v + w, v − w) ∈ Y1 . Therefore, by (3), (v + w, v − w) ∈ Y2 . But 2 2 µ2 (v + w, v − w) = v2 − w2 = a2 − b2 ∈ R {0}, and so we have 2 a contradiction, establishing the claim. Set y = v − v1 µ1 (v, w)−1 w. 2 2 Then µ1 (y, v) = v1 − rµ1 (v, w) = 0, where r = v1 µ1 (v, w)−1 , and so (y, v) ∈ Y1 ⊆ Y2 . Since the set {v, w} is linearly independent, we know −1 that y = 0V . If we set y = y1 y, then (y , v) ∈ Y1 ⊆ Y2 and so, as 2 2 before, µ1 (y + v, y − v) = y 1 − v1 = 0. Hence (y + v, y − v) ∈ Y1 . 2 2 2 2 4 −2 2 Thus y1 + v1 = −y + v1 = rw1 = v1 |µ1 (v, w)| w1 and so 2 4 −2 2 2 y1 = v1 |µ1 (v, w)| w1 − v1 . Since µ2 (y, v) = 0, we see that 2

2

2

2

4

2

2

y2 + v2 = −y + v2 = rw2 = v1 |µ1 (v, w)|

−2

and so 2

y2

4

−2

4

−2

=

v1 |µ1 (v, w)|

=

v1 |µ1 (v, w)| b2 w1 − a2 v1 4 −2 2 2 2 a2 v1 |µ1 (v, w)| w1 − v1 = a2 y1 .

>

w2 − v2 2

2

Since µ2 (y , v) = 0, this implies that µ2 (y + v, y − v) = y 2 − v2 > a2 − a2 = 0, 2

2

2

w2

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16. Orthogonality

contradicting (3) and the fact that µ1 (y + v, y − v) = 0. From this contradiction, we conclude that there can be no elements a and b as 2 2 above, so there must exist a positive real number c such that v2 = c v1 for each nonzero vector v ∈ V. Then for each v, w ∈ V we have µ2 (v, w)

= =

which proves (1).

1 [v + w2 − v − w2 ] 4 c2 [v + w1 − v − w1 ] = c2 µ1 (v, w), 4

Let V be an inner product space. We have already seen that, for each w ∈ V, the function from V to the field of scalars given by v → v, w belongs to D(V ). If V is finitely generated, we claim that every element of D(V ) is of this form. The following result is actually a special case of a much wider, and more complicated, theorem. (16.13) Proposition (Riesz5 Representation Theorem): Let V be a finitely-generated inner product space. If δ ∈ D(V ) then there exists a unique vector y ∈ V satisfying δ(v) = v, y for all v ∈ V. Proof: Let {v1 , . . . , vn } be an orthonormal basis for V n y = i=1 δ(vi )vi . Then for all 1 ≤ h ≤ n we have 9 8 n n δ(vi )vi = δ(vi ) vh , vi = δ(vh ) vh , y = vh , i=1

and let

i=1

and so v, y = δ(v) for all v ∈ V. The vector y is unique since if n n v, x = v, y for all v ∈ V then x = i=1 x, vi vi = i=1 δ(vi )vi = y, as desired. Example: Let n > 1 be an integer and let V be the subspace of RR consisting of all polynomial functions of degree 4 1 at most n, on which we have an inner product defined by f, g = −1 f (t)g(t)dt. Let δ ∈ D(V ) be the linear functional defined by δ : f → f (0). By Proposition

5

The 20th century Hungarian mathematician Frigyes Riesz was one of the founders of functional analysis.

16. Orthogonality

339

16.13, there 4 1 exists a polynomial function p ∈ V satisfying the condition f (0) = −1 f (t)p(t)dt for all f ∈ V. The function p is defined to be n i=0 pi (0)pi , where pi is the ith Legendre polynomial. (16.14) Proposition: Let V and W be finitely-generated inner product spaces, and let α : V → W be a linear transformation. Then there exists a unique linear transformation α∗ : W → V satisfying the condition α(v), w = v, α∗ (w) for all v ∈ V and all w ∈ W. Proof: Let w be a given vector in W. It is easy to check that the function δ from V to F defined by δ : v → α(v), w is a linear functional. By Proposition 16.13, we know that there exists a unique vector yw ∈ V satisfying δ(v) = v, yw for all v ∈ V. Define the function α∗ : W → V by α∗ : w → yw . We have to prove that this function is indeed a linear transformation. Indeed, if w1 , w2 ∈ W then v, α∗ (w1 + w2 )

= α(v), w1 + w2 = α(v), w1 + α(v), w2 = v, α∗ (w1 ) + v, α∗ (w2 ) = v, α∗ (w1 ) + α∗ (w2 )

and this is true for all v ∈ V, we have α∗ (w1 + w2 ) = α∗ (w1 ) + α∗ (w2 ) for all w1 , w2 ∈ W. If c is a scalar and if w ∈ W then v, α∗ (cw) = α(v), cw = c α(v), w = c v, α∗ (w) = v, cα∗ (w) for all v ∈ V, and hence α∗ (cw) = cα∗ (w). Thus α∗ is a linear transformation and, since yw is uniquely defined, it is also unique. Let V and W be inner product spaces and let α : V → W be a linear transformation. A linear transformation α∗ : W → V satisfying the condition α(v), w = v, α∗ (w) for all v ∈ V and w ∈ W is called an adjoint transformation of α. By Proposition 16.14, we know that if V and W are finitely generated then every α ∈ Hom(V, W ) has a unique adjoint. (16.15) Proposition: Let V and W be finitely-generated inner product spaces, having orthonormal bases B = {v1 , . . . , vn } and D = {w1 , . . . , wk } respectively. Let α : V → W be a linear transformation. Then ΦBD (α) is the matrix A = [aij ], where aji = α(vi ), wj and ΦDB (α∗ ) = AH . k Proof: For all 1 ≤ i ≤ n, let α(v Ci ) = h=1 ahjDwh . Then for all k = aji and also 1 ≤ j ≤ k we have α(vi ), wj = h=1 ahj wh , wj α∗ (wj ), vi = vi , α∗ (wj ) = α(vi ), wj = aji , which is what we needed.

340

16. Orthogonality

Example: It is of course possible that a linear transformation between inner product spaces can have an adjoint even if the spaces are not finitely generated. For example, let [a, b] be a closed interval on the real line and let V be the vector space of all differentiable functions from [a, b] to R. 4b Define an inner product on V by setting f, g = a f (x)g(x)dx. This is an inner product space which is not finitely generated over R. Let α 4b be the endomorphism of V satisfying α(f ) : x → a e−tx f (t)dt. Then α(f ), g = f, α(g) for all f, g ∈ V, and so α∗ exists, and equals α. (16.16) Proposition: Let V, W, and Y be inner product spaces. Let α and β be linear transformations from V to W having adjoints, let ζ be a linear transformation from W to Y having an adjoint, and let c be a scalar. Then: (1) (α + β)∗ = α∗ + β ∗ ; (2) (cα)∗ = cα∗ ; (3) (ζα)∗ = α∗ ζ ∗ ; (4) α∗∗ = α. Proof: (1) For all v ∈ V and all w ∈ W , we have v, (α + β)∗ (w)

= (α + β)(v), w = α(v) + β(v), w = α(v), w + β(v), w = v, α∗ (w) + v, β ∗ (w) = v, (α∗ + β ∗ )(w)

and so by the uniqueness of the adjoint we get (α + β)∗ = α∗ + β ∗ . (2) For all v ∈ V and all w ∈ W , we have v, (cα)∗ (w)

= (cα)(v), w = c(α(v)), w = c α(v), w = c v, α∗ (w) = v, cα∗ (w) = v, (cα∗ )(w)

and so (cα)∗ = cα∗ . (3) For all v ∈ V and all y ∈ Y , we have v, (ζα)∗ (y) = (ζα)(v), y = α(v), ζ ∗ (y) = v, α∗ ζ ∗ (y) and so (ζα)∗ = α∗ ζ ∗ . (4) For all v ∈ V and all w ∈ W , we have w, α∗∗ (v) = α∗ (w), v = v, α∗ (w) = α(v), w = w, α(v) and so α∗∗ = α.

For a finitely-generated inner product space V, we can consider the assignment α → α∗ as a function from End(V ) to itself which satisfies the following conditions: (1) σ ∗1 = σ 1 ;

16. Orthogonality

341

(2) (α + β)∗ = α∗ + β ∗ and (αβ)∗ = β ∗ α∗ for all α, β ∈ End(V ); (3) α∗∗ = α for all α ∈ End(V ). A function satisfying these conditions is called an involution on the F algebra End(V ). Another involution we have already seen is the function A → AT on the F -algebra Mn×n (F ), for any field F. Of course, in the case F = R, the relation between these two involutions can be seen from Proposition 16.15. We have also seen that the function A → AH is an involution of Mn×n (C), and its relation to the involution α → α∗ is also immediate from Proposition 16.15. (16.17) Proposition: Let α : V → W be a linear transformation between finitely-generated inner product spaces. Then: (1) ker(α∗ ) = im(α)⊥ ; (2) ker(α) = im(α∗ )⊥ ; (3) im(α) = ker(α∗ )⊥ ; (4) im(α∗ ) = ker(α)⊥ . Proof: (1) We note that ker(α∗ ) = {w ∈ W | α∗ (w) = 0V } = {w ∈ W | v, α∗ (w) = 0 for all v ∈ V } = {w ∈ W | α(v), w = 0 for all v ∈ V } = im(α)⊥ . α∗ .

(2) This follows from the same argument as (1), replacing α by

(3) By (1) and Proposition 16.6, we have im(α) = (im(α)⊥ )⊥ = ker(α∗ )⊥ . (4) This follows from (2) in the same way (3) follows from (1). (16.18) Proposition: If α is an endomorphism of a finitelygenerated inner product space V then null(α) = null(α∗ ). Proof: By Proposition 6.10 and Proposition 16.17, we know that null(α) = dim(im(α∗ )⊥ ) = dim(V ) − dim(im(α∗ )) = null(α∗ ) and so we are done.

Example: Proposition 16.18 is not necessarily true for inner product spaces which are not finitely generated. For example, let V = R(∞) with ∞ the inner product [a0 , a1 , . . .], [b0 , b1 , . . .] = i=0 ai bi . Let α ∈ End(V ) be given by α : [a0 , a1 , . . .] → [0, a0 , a1 , . . .]. Then α∗ exists and is given by α∗ : [a0 , a1 , . . .] → [a1 , a2 , . . .]. Clearly, ker(α) is trivial but ker(α∗ ) is not.

342

16. Orthogonality

(16.19) Proposition: Let α : V → W be a linear transformation between finitely-generated inner product spaces. Then (1) If α is a monomorphism then α∗ α is an automorphism of V ; (2) If α is an epimorphism then αα∗ is an automorphism of W. Proof: (1) It suffices to prove that the linear transformation α∗ α is monic. And, indeed, if v ∈ V satisfies α∗ α(v) = 0V then α(v), α(v) = α∗ α(v), v = 0V , v = 0 and so α(v) = 0W . Since α is a monomorphism, v = 0V and so we have shown that α∗ α is monic, as we needed. (2) First of all, we will show that α∗ is a monomorphism. Indeed, if w1 , w2 ∈ W are vectors satisfying α∗ (w1 ) = α∗ (w2 ) then for all v ∈ V we have α(v), w1 − w2 = v, α∗ (w1 ) − α∗ (w2 ) = 0 and since α is an epimorphism, we conclude that w, w1 − w2 = 0 for all w ∈ W. This implies that w1 − w2 = 0V and so w1 = w2 , showing that α∗ is indeed monic. Now we will show that αα∗ is also monic, which will suffice to prove (2). Indeed, if αα∗ (w) = 0W then α∗ (w), α∗ (w) = αα∗ (w), w = 0 and so α∗ (w) = 0V , proving that w = 0W . (16.20) Proposition: Let α : V → W be an isomorphism be∗ −1 tween −1 ∗ finitely-generated inner produce spaces. Then (α ) = α . ∗ LetF β = α−1 . Then for all v1 , v2 ∈ V we have v1 , v2 = E Proof: α−1 α(v1 ), v2 = α(v1 ), β(v2 ) = v1 , α∗ β(v2 ) and so α∗ β(v2 ) = v2 for all v2 ∈ V, which means that α∗ β is the identity map on V. Thus β = (α∗ )−1 . Finally, we note that in an inner product space over R we can also project onto affine subsets and not just onto subspaces. Indeed, if V is an inner product space over R then any element v of V defines a linear functional δ v ∈ D(V ) given by δ v : w → w, v . If 0 = c ∈ R, then δ −1 c (c) is an affine subset of V . Define a function θ v : V → V by setting c − δ v (y) θv : y → y + v. 2 v Then for all y ∈ V we have δ v θv (y) = c and so we see that θv (y) ∈ δ −1 c (c), 2 (c). Moreover, θ = θ . We call the function θv so that im(θv ) ⊆ δ −1 v c v the projection on the affine set δ −1 (c). Such projections have many c applications, such as the algebraic reconstruction technique (ART), which is very important in computerized imaging.

16. Orthogonality

343

Exercises

Exercise 904 Let A =

2 1

B ∈ M2×2 (R) of the form

1 2

! ∈ M2×2 (R). Does there exist a matrix cos(t) sin(t)

− sin(t) cos(t)

! such that the columns

of A + B are orthogonal, when considered as elements of the space R2 , endowed with the dot product? 

   2 3 Exercise 905 Calculate the angle between the vectors  1  and  1  1 −2 3 in the space R , endowed with the dot product.    Exercise 906 Calculate the angle between the vectors   

1 1 1 2 1





     and     

1 −1 1 −1 1

     

in the space R5 , endowed with the dot product. Exercise 907 Let A and B be nonempty subsets of R3 which satisfy the condition that u × v ∈ B whenever u ∈ A and v ∈ B. Is it true that u × w ∈ B ⊥ whenever u ∈ A and w ∈ B ⊥ . Exercise 908 Let V = M2×2 (R) and define an inner product on V ! !H G 2 2 b11 b12 a11 a12 , = i=1 j=1 aij bij . Find the by setting a21 a22 b21 b22 ! ! 1 1 1 1 angle between the matrices and . 1 1 −1 1 Exercise 909 Let V = C(0, 1) on which we have defined the inner prod41 uct f, g = 0 f (x)g(x)dx. Calculate cos(t) . Exercise 910 Let V be the space R4 , together with the dot product. Find a normal vector in V which is orthogonal to each of the vectors       1 1 2  1   −1   1   ,      1   −1  , and  1  . 1 1 3

344

16. Orthogonality

Exercise 911 Let V = R3 on which some inner product is defined. Does there exist a vector 0V = v ∈ V which is orthogonal to each of the vectors       2 1 2  1  ,  −1  , and  0 ? 3 1 4 Exercise 912 Let f, g ∈ RR be defined by f : x → x and g : x → x2 − 12 . Are f and g orthogonal as elements of C(0, 1)? Are they orthogonal as elements of C(0, 2)? Exercise 913 Find a real number c such that v − w = c for every orthonormal pair {v, w} of vectors in Rn , on which the dot product is defined. Exercise 914 Let n be a positive integer and let c1 , . . . , cn is a list n of real numbers. Let {v1 , . . . , vn } be an orthonormal basis √ for R , let d = min{c1 , . . . , cn }. For each 1 ≤ i ≤ n, set di = ci − d and let wi = dvi . Let B ∈ Mn×n (R) be the matrix the columns of which are d1 , . . . , dn and let A = BB T + dI. For 1 ≤ i ≤ n, show that vi is an eigenvector of A associated with the eigenvalue ci . Exercise 915 Let V = C(0, 1) on which we have defined the inner prod41 uct f, g = 0 f (x)g(x)dx, and let W = R{ex } ⊆ V. Find an infinite set of elements of W ⊥ . Exercise 916 Let V = R4 on which some inner product is defined. Find distinct vectors v, w, y ∈ V such that v ⊥ w and w ⊥ y, but not v ⊥ y. Exercise 917 Let V be an inner product space over R and let v and w be vectors in V. Show that v = w if and only if (v +w) ⊥ (v −w). Exercise 918 Let V = C(−1, 1) and define an inner product on V by 41 setting f, g = −1 f (x)g(x)dx. Let W be the subspace of V composed of all even functions. Find W ⊥ . Exercise 919 Let n be a positive integer and let V = Mn×n (C), on which we have an inner product defined by A, B = tr(AT B). Let W be the subspace of V consisting of all those matrices A ∈ V satisfying tr(A) = 0. Find W ⊥ . Exercise 920 Let V be an inner product space having subspaces W and Y. Show that (W + Y )⊥ = W ⊥ ∩ Y ⊥ . Exercise 921 !Define an inner product on R2 with respect to which the ! −1 2 vectors and are orthogonal. 2 4

16. Orthogonality

345

Exercise 922 Make use of the Gram-Schmidt process to find an orthonormal basis for the space R3 together with the dot product, beginning with       1 1   1  1  ,  −2  ,  2  . the initial basis   1 1 3 Exercise 923 Let V be an inner product space and let A be an orthonormal subset of V. Show that A is a maximal orthonormal subset if and only if for every 0V = y ∈ V there exists a v ∈ A satisfying v, y = 0. Exercise 924 Let V be an inner product space of finite dimension n over its field of scalars. Show that there exists a subset {v1 , . . . , v2n } of V satisfying the conditions that vi , vj ≤ 0 for all 1 ≤ i = j ≤ 2n. Exercise 925 Let V be the space of all polynomial 4functions in RR of 1 degree less than 3, with inner product p, q = 12 −1 p(t)q(t)dt. Find an orthonormal basis {p0 , p1 , p2 } of V satisfying deg(ph ) = h for h = 0, 1, 2. Exercise 926 Consider the function µ : R3 × R3 → R given by     a a µ :  b  ,  b  → 2aa + ac + ca + bb + cc . c c Show that µ is an inner product and find a basis of R3 orthonormal with respect to µ. Exercise 927 Let V be an inner product space over R and let W be a finitely-generated subspace of V with orthonormal basis {w1 , . . . , wn }. n Let α ∈ Hom(V, W ) be defined by α : v → i=1 v, wi wi . Show that α(v) − v ∈ W ⊥ for all v ∈ V and that α(v) − v < w − v for all α(v) = w ∈ W. Exercise 928 Let  1     2 dent subset  0    3

W be the subspace of R4 spanned by linearly-indepen     4 8     0   1  , ,  , which is an inner product space   5   5    8 6

with respect to the dot product. Make use of the Gram-Schmidt process to find an orthonormal basis for W. Exercise 929 Let n be a positive integer and let A ∈ Mn×n (R). If the set of rows of A is orthonormal with respect to the dot product, is the same true for the set of columns of A?

346

16. Orthogonality

Exercise 930 Let n > k be positive integers and let A ∈ Mk×n (R) satisfy the condition that its set of rows is orthonormal with respect to the dot product. Show that (AT A)2 = AT A. Exercise 931 Let n be a positive integer and let A ∈ Mn×n (R). Show that A is symmetric if and only if for some k < n there exists a matrix B ∈ Mn×k (R) and a real number r such that A = BB T + rI and the columns of B are mutually orthogonal. Exercise 932 Let W be the subspace of R4 , which is an inner product space with respect to the dot product, generated by         2 0 4 1          2   1  1 0  , , ,  .  0   1   2   1       0 2 4 1 Find an orthonormal basis for W and an orthonormal basis for W ⊥ . Exercise 933 Consider R4 as an inner product space with     1 1   1   1 1 1  ,  dot product. Add two vectors to the set  6 3  2 1   −5 1 to get an orthonormal basis for this space.

respect to the       in order  

Exercise 934 Let n be a positive integer and let V = Rn , which is an inner product space with respect to the dot product. Let {v1 , . . . , vn } be an orthonormal basis for V, let a ∈ R, and let 1 ≤ h = k ≤ n. Define vectors w1 , . . . , wn in V by setting   cos(a)vh − sin(a)vk if i = h sin(a)vh − cos(a)vk if i = k . wi =  otherwise vi Is {w1 , . . . , wn } an orthonormal basis for V ? Exercise 935 Consider R3 as an inner product space with respect to the dot product. Does there exist an integer k such that       0 −25   4k  4  ,  k  ,  16k    −k 4 −12k is an orthonormal basis for this space.

16. Orthogonality

347

Exercise 936 Consider R4 as an inner product space with respect to the       1 1 0           0 1 , , 1  . dot product. Find an orthonormal basis for R   1   2   1       0 1 2 Exercise 937 Define an inner product on R2 by setting G ! !H 1 a c , = ac + (ad + bc) + bd. b d 2 Find an orthonormal basis for this space. Exercise 938 Consider R3 as an inner product space with respect to the dot product. Let a, b, c, d be nonzero real numbers satisfying the conditions that a2 + b2 + c2 = d2 and ab + ac = bc. Show that the subset        b c  1 a  b  , 1  −c  , 1  a  of R3 is orthonormal.  d d d c a −b Exercise 939 Define an inner product on R3 by setting  8 a   b1 9 1  a2  ,  b2  = a1 b1 + 2(a2 b2 + a3 b3 ) − (a1 b2 + a2 b1 ) − (a2 b3 + a3 b2 ). a3 b3 Find an orthonormal basis for this space. Exercise 940 Let m be a positive integer and let W = {f ∈ CZ | f (i + m) = f (i) for all i ∈ Z}, which is a subspace of the vector space CZ over m−1C. Define a function µ : W × W → C by setting µ : (f, g) → h=0 f (h)g(h). For each 0 ≤ j < m, let fj ∈ W be the function defined by

1 if h is of the form j + mi, for i ∈ Z . fj (h) = 0 otherwise Show that µ is an inner product on W and that, with respect to that product, {f0 , . . . , fm−1 } is an orthonormal basis for W. Exercise 941 A function f ∈ RR has bounded support if and only if there exist real numbers a ≤ b such that f (x) = 0 for all x not in the interval [a, b] on the real line. Let V be the set of all such 4 ∞functions and define a function µ : V × V → R by setting µ (f, g) = −∞ f (x)g(x)dx. For each k ∈ Z, let fk ∈ V be the function defined by

1 if k ≤ x ≤ k + 1 fk : x → . 0 otherwise

348

16. Orthogonality

Show that µ is an inner product on V and that the subset {fk | k ∈ Z} of V is orthonormal with respect to this inner product. Exercise 942 Let V be the subspace of RR consisting of all infinitelydifferentiable functions f which are periodic of period h > 0. (In other words, f (x + h) = f (x) for all x ∈ R). Define an inner product on V 4h by setting f, g = −h f (x)g(x)dx. Let α be the endomorphism of V which assigns to every element of V its derivative. Find α∗ . Exercise 943 Let V be an inner product space over R and let {v1 , . . . vn } . . . , an be be a set of mutually-orthogonal nonzero n vectors in V. Let a1 , n a = 1, and let w = positive real numbers satisfying i=1 i i=1 ai vi . Suppose that w ⊥ vi − vj for all 1 ≤ i = j ≤ n. Then show that n −2 −2 w = i=1 vi . Exercise 944 Let V be a finitely-generated inner product space and let α, β 1 , β 2 ∈ End(V ) satisfy α∗ αβ 1 = α∗ αβ 2 . Show that αβ 1 = αβ 2 .

17 Selfadjoint Endomorphisms

Let V be an inner product space. An endomorphism α of V is selfadjoint if and only if α(v), w = v, α(w) for all v, w ∈ V. Such endomorphisms always exist since σ c is selfadjoint for any c ∈ R. Selfadjoint endomorphisms have important applications in mathematical models in physics. For example, in mathematical models of quantum theory, selfadjoint operators on the state space of a system represent measurements which can be performed on the system. Note that if α ∈ End(V ) is selfadjoint, then α(v), v = v, α(v) = α(v), v and so α(v), v ∈ R for all v ∈ V. Example: Let V = C(0, 1), which is an inner product space over R in 41 which f, g = 0 f (x)g(x)dx. Then the endomorphism α of V defined 41 by α(f ) : x → 0 cos(x − y)f (y)dy for all f ∈ V is selfadjoint. (17.1) Proposition: Let V be an inner product space. Then: (1) If α ∈ End(V ) has an adjoint α∗ , then α+α∗ is self-adjoint; (2) If α ∈ End(V ) is selfadjoint, so is cα for each c ∈ R; (3) If α ∈ End(V ) is selfadjoint, so is αn for each positive integer n; (4) If α, β ∈ End(V ) are selfadjoint so are α + β and α • β, where • is the Jordan product in End(V ); (5) If α ∈ End(V ) is selfadjoint and β ∈ End(V ) has an adjoint, then βαβ ∗ is selfadjoint. 349

350

17. Selfadjoint Endomorphisms

Proof: (1). If v, w ∈ V then (α + α∗ )(v), w

= α(v), w + α∗ (v), w = v, α∗ (w) + v, α(w) = v, (α + α∗ )(w) .

(2) If v, w ∈ V then (cα)(v), w = c α(v), w = c v, α(w) = v, (cα)(w) . (3) This follows by an easy induction argument, using Proposition 16.16(3). (4) The selfadjointness of α + β is an immediate consequence of Proposition 16.16(1). Also, recall that α • β = 12 (αβ + βα) and so, if v, w ∈ V then ( α • β)(v), w

= =

1 αβ(v), w + 2 1 v, βα(w) + 2

1 βα(v), w 2 1 v, αβ(w) = v, ( α • β)(w) . 2

(5) By Proposition 16.16, we see that (βαβ ∗ )∗ = β ∗∗ αβ ∗ = βαβ ∗ . In particular, if α is a selfadjoint endomorphism of an inner product space V, and if p(X) ∈ R[X], then p(α) is selfadjoint. The product of selfadjoint endomorphisms of V need not be selfadjoint, as we will see in the example after Proposition 17.4. Example: Let V be an inner product space over R and let α ∈ End(V ) be selfadjoint. Let a, b ∈ R satisfy the condition that a2 < 4b. Then, by the previous remark, we know that β = α2 + aα + bσ 1 is again a selfadjoint endomorphism of V. Moreover, if 0V = v ∈ V then E F β(v), v = α2 (v), v + a α(v), v + b v, v = α(v), α(v) + a α(v), v + b v, v =

2

2

α(v) + a α(v), v + b v .

By Proposition 15.2, we know that |α(v), v| ≤ α(v) · v and so β(v), v

≥ =

2

2

α(v) − |a| · α(v) · v + b v 2 1 1 2 α(v) − |a| · v + b − a2 v > 0. 2 4

Thus β(v) = 0V for each 0V = v ∈ V, showing that β is monic. In particular, if V is finitely generated, this in fact shows that β is an automorphism of V.


351

Let V be a finitely-generated inner product space having an orthonormal basis D. If α ∈ End(V ) and if ΦDD (α) = [aij ], then we know from Proposition 16.15 that ΦDD (α∗ ) = ΦDD (α)H = [aij ]T . Therefore, if α is selfadjoint we have aij = aji for all 1 ≤ i, j ≤ n. In particular, aii = aii for all 1 ≤ i ≤ n and so the diagonal entries in ΦDD (α) belong to R. Matrices A over C satisfying the condition that A = AH are known as Hermitian matrices. When we are working over R, these are of course just the symmetric matrices. It is clear that the sum of Hermitian matrices is again a Hermitian matrix, but the product of Hermitian matrices is not necessarily Hermitian, just as we have seen that the product of symmetric matrices is not necessarily symmetric. We do note, however, that if a matrix A ∈ Mn×n (C) is Hermitian then so is A2 . Indeed, if A and B are Hermitian matrices in Mn×n (C), then their Jordan product 12 (AB + BA) is a Hermitian matrix and so, in particular, the product of a commuting pair of Hermitian matrices is again Hermitian. Moreover, any matrix D ∈ Mn×n (C) can be written in the form A + iB, where A = 12 (D + DH ) and B = − 21 (D − DH ) are both Hermitian matrices. If A ∈ Mn×n (C) is Hermitian, then so is cA for any c ∈ R, and so the set of all Hermitian matrices in Mn×n (C) is a subspace of Mn×n (C), considered as a vector space over R; indeed, it is a subalgebra of the commutative Jordan R-algebra Mn×n (C)+ . However, this set is not closed under multiplication by complex scalars, and so it is not a vector space over C. We have already seen that if V is an inner product space and if α ∈ End(V ) is selfadjoint, then α(v), v ∈ R for all v ∈ V. If V is finitely generated, the reverse is also true, as follows immediately from the following result. (17.2) Proposition: Let V be an inner product space over C and let α ∈ End(V ) have an adjoint. If α(v), v ∈ R for all v ∈ V , then α is selfadjoint. Proof: For vectors v, w ∈ V, we have α(v + w), v + w) = α(v), v + α(v), w + α(w), v + α(w), w and since, by assumption, we know that the scalars α(v + w), v + w) , α(v), v , and α(w), w are all real, we see that α(v), w+α(w), v ∈ R as well. This implies that α(v), w + α(w), v = w, α(v) + v, α(w) and so i α(v), w + i α(w), v = i w, α(v) + i v, α(w) . Similarly, α(v + iw), v + iw) = α(v), v − i α(v), w + i α(w), v + α(w), w

352


and so −i α(v), w + i α(w), v ∈ R. This implies that −i α(v), w + i α(w), v = i w, α(v) − i v, α(w) and so, multiplying by i and adding it to the previous result, we get 2 α(v), w = 2 w, α(v) , whence α(v), w = w, α(v) . Therefore α = α∗ . (17.3) Proposition: Let V be an inner product space and let σ 0 = α ∈ End(V ) be selfadjoint. Then there exists a vector v ∈ V satisfying α(v), v = 0. Proof: First assume that the field of scalars is C. Then it is easy to check that if v, w ∈ V then α(v), w

1 4

=

[α(v + w), v + w − α(v − w), v − w]

+ 4i [α(v + iw), v + iw − α(v − iw), v − iw] . Moreover, each term on the right-hand side of this equality is of the form α(y), y for some y ∈ V, so if all of these were equal to 0 we would see that α(v) ⊥ w for all v, w ∈ V, which means that α(v) = 0V for all v ∈ V, contradicting the hypothesis that σ 0 = α. Thus the desired result must hold. Now assume that the field of scalars is R. Then for all v, w ∈ V we have α(w), v = w, α(v) = α(v), w and so α(v), w =

1 4

[α(v + w), v + w − α(v − w), v − w] .

Again, each term on the right-hand side of this equality is of the form α(y), y for some y ∈ V so if all of these were all equal to 0 we would have α(v) ⊥ w for all v, w ∈ V which, as we have seen in the previous case, leads to a contradiction. We now return to a new variant of a question we have already posed: if α is an endomorphism of an inner product space V, when does there exist an orthonormal basis of V composed of eigenvectors of α? If such a basis exists, we say that α is orthogonally diagonalizable. (17.4) Proposition: Let V be an inner product space and let α ∈ End(V ) be selfadjoint. Then spec(α) ⊆ R and eigenvectors of α associated with distinct eigenvalues are orthogonal.

Proof: Let c be an eigenvalue of α and let v be an eigenvector of α associated with c. Then c v, v = cv, v = α(v), v = v, α(v) =


353

v, cv = c v, v and so, since v = 0V , we see that c = c, proving that c ∈ R. Thus we have shown the first assertion. If c and d are distinct eigenvalues of α associated with eigenvectors v and w respectively, then c v, w = cv, w = α(v), w = v, α(w) = v, dw = d v, w . Since c = d, this implies that v, w = 0. Example: The endomorphisms α and β of C2 which are given by ! ! ! ! a b a a α: → and β : → can easily be seen to be b a b −b selfadjoint. However, spec(βα) = {i, −i} and so, by Proposition 17.4, βα is not selfadjoint. We note the following consequence of Proposition 17.4: if the matrix A ∈ Mn×n (R) is symmetric, then all eigenvalues of A are real, and so the characteristic polynomial of A is completely reducible in R[X]. By Proposition 17.4 we see that if V is an inner-product space of finite dimension n over C and if α ∈ End(V ) is selfadjoint, then the eigenvalues of α can be written uniquely as an n-tuple (c1 (α), . . . , cn (α)) of real numbers, the entries of which form a nonincreasing sequence. Weyl showed that if α, β ∈ End(V ), if 1 ≤ k ≤ i ≤ n, and 1 ≤ j ≤ n − i + 1, then ci+j−1 (α) + cn−j+1 (β) ≤ ci (α + β) ≤ ci−k+1 (α) + ck (β) and so, if j = k = 1, we have ci (α) + cn (β) ≤ ci (α + β) ≤ ci (α) + c1 (β) for each 1 ≤ i ≤ n. In particular, c1 (α + β) ≤ c1 (α) + c1 (β) and cn (α) + cn (β) ≤ cn (α + β). We now turn to the problem of finding the eigenvalues of a selfadjoint endomorphism of a finitely-generated inner product space. This problem arises in many important applications. For example, let Γ be a (nondirected) graph with vertex set {1, . . . , n}. We associate to this graph a symmetric matrix, called the adjacency matrix [aij ], the entries of which are nonnegative integers, by setting aij to be the number of edges in Γ connecting vertex i to vertex j. The matrix represents a selfadjoint endomorphism of Rn with respect to some basis and its spectrum can be used to derive important information about Γ. This technique has important applications in the analysis of computer networks and in such areas as chemistry, where it is used to make rough estimates of the electron density distribution of molecules. (17.5) Proposition: If V is a nontrivial finitely-generated inner product space, then spec(α) = ∅ for any selfadjoint endomorphism α of V. Proof: Let α be a selfadjoint endomorphism of V. Choose an orthonormal basis B = {v1 , . . . , vn } for V and let A = ΦBB (α). Since

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α is selfadjoint, we know that A = AH . Let W = Cn on which we have defined the dot product. Then the endomorphism β of W defined by β : w → Aw is selfadjoint. The degree of the characteristic polynomial |XI − A| of β is n > 0 and so, by the Fundamental Theorem of Algebra, it has a root c ∈ C. Thus the matrix cI − A is singular and so there exists a nonzero vector w ∈ W satisfying Aw = cw. In other words, c ∈ spec(β). By Proposition 17.4, this implies that c ∈ R and so c ∈ spec(α), even if V is an inner product space over R. In particular, we learn from Proposition 17.5 that every symmetric matrix over R has an eigenvalue. Compare this to the example we have already seen of a symmetric matrix in M2×2 (GF (2)) having no eigenvalues. Let V be an inner product space finitely generated over C and let α be a selfadjoint endomorphism of V . We know, by Proposition 17.4, that the eigenvalues of α are all real and that eigenvectors of α associated with distinct eigenvalues are orthogonal. Let us denote the eigenvalues of α by c1 , . . . , cn where the indices are so chosen that c1 ≥ . . . ≥ cn . An important result known as the CourantFischer Minimax Theorem states that, for each 1 ≤ k ≤ n, we have ck = sup {inf{α(w), w | w ∈ W and w = 1}} , where the supremum runs over all subspaces W of V having dimension k. Let us look at this from a different perspective. The function which −2 assigns to each 0V = v ∈ V the scalar Rα (v) = v, α(v) v is called 1 the Rayleigh quotient function. Note that the projection π v defined in connection with the Gram-Schmidt theorem satisfies the condition that π v : α(v) → Rα (v)v. By what we have already seen, the image D of this function is contained in R. Moreover, if v is an eigenvector of α with associated eigenvalue c, then Rα (v) = c, and so ∅ = spec(α) ⊆ D. On the other hand, it is possible to show – though we will not do it here – that D is contained in the closed interval [cn , c1 ] bounded by the largest

1 Twentieth-century German mathematicians Ernst Fischer and Richard Courant studied spaces of functions. Courant, who headed the Mathematics Institute at the University of G¨ ottingen, fled Germany in 1933 and founded a similar institute in New York City, which now bears his name. John William Strutt, Lord Rayleigh, was a 19th-century British physicist and applied mathematician, who made important contributions to mathematical physics and who won the Nobel prize in 1904 for his discovery of the inert gas argon.


355

and the smallest eigenvalues of α, both endpoints of which in fact belong to D. This observation can be used to define the Rayleigh quotient iterative scheme to find eigenvalues of a selfadoint endomorphism α:

As an initial guess, choose a normal vector v0 and let d0 = Rα (v0 ). For k = 0, 1, 2, . . . repeat the following steps: / Aut(V ), then dk is an eigenvalue of α, (1) If α − dk σ 1 ∈ and we are done; (2) Otherwise, α−dk σ 1 ∈ Aut(V ). Set y = (α−dk σ 1 )−1 (vk ) −2 and then compute vk+1 = y y and dk+1 = Rα (vk+1 ). This scheme will indeed produce an eigenvalue of α for all guesses of v0 except those in a set of measure 0, and when it converges, the convergence is very rapid. Its main disadvantage is the time and effort needed in step (1) of the iteration, to decide if α − dk σ 1 is an automorphism of V or not (usually, if the matrix representing this endomorphism is nonsingular or not) and, if it is, to compute its inverse; the algorithm is therefore worthwhile only if this can be done without major computational effort. Example: Let α be the endomorphism of R3 represented with respect   2 1 1 to the canonical basis by the symmetric matrix A =  1 3 1  . Then 1 1 4   1 1 α is selfadjoint. Choose v0 = √  1  . Using the above algorithm, we 3 1 see that d0 = Rα (v0 ) = 5, which is not an eigenvalue of α. Moreover,   0.3841106399 . . . v1 =  0.5121475201 . . .  and d1 = 5.213114754 . . . 0.7682212801 . . .   0.3971170680 . . . v2 =  0.5206615990 . . .  and d2 = 5.214319743 . . . 0.7557840528 . . . The actual value of an eigenvalue of α is 5.214319744 . . . , so we see that convergence was very rapid indeed. (17.6) Proposition: Let V be a finitely-generated inner product space and let α ∈ End(V ). If W is a subspace of V invariant under α, then W ⊥ is invariant under α∗ .

356


Proof: If w ∈ W and y ∈ W ⊥ . Then α(w) ∈ W and so w, α∗ (y) = α(w), y = 0, whence α∗ (y) ∈ W ⊥ . If V is a nontrivial inner product space finitely generated over R and assume that α ∈ End(V ) is orthogonally diagonalizable. Then there exists an orthonormal basis B = {v1 , . . . , vn } composed of eigenvectors of α. Thus ΦBB (α) is a diagonal matrix and so symmetric. In particular, ΦBB (α∗ ) = ΦBB (α)T = ΦBB (α), which proves that α = α∗ and so α is selfadjoint. The converse of this result follows from the following Proposition. (17.7) Proposition: Let V be a nontrivial finitely-generated inner product space and let α ∈ End(V ) be selfadjoint. Then α is orthogonally diagonalizable. Proof: We will prove the result by induction on n = dim(V ). For n = 1, we know y Proposition 17.5 that α has an eigenvector v ∈ V, −1 and so {v1 } is the desired basis, where v1 = v v. Now assume that n > 1 and that the proposition has been established for all spaces of dimension less than n. Pick v1 as before and let W be the subspace of V generated by {v1 }. Then V = W ⊕ W ⊥ and, by Proposition 17.6, we know that W ⊥ is invariant under α∗ = α. Moreover, W ⊥ is an inner product space of dimension n − 1 and the restriction of α to W ⊥ is selfadjoint. Therefore, by the induction hypothesis, there exists an orthonormal basis {v2 , . . . , vn } of W ⊥ composed of eigenvectors of α. Since v1 is orthogonal to each of the vectors in this basis, we see that {v1 , . . . , vn } is an orthonormal basis of V. Let V be an inner product space. An endomorphism α ∈ End(V ) is positive definite if and only if it is selfadjoint and satisfies the condition that α(v), v is a positive real number for all 0V = v ∈ V. Thus we see that σ c is positive definite for any positive real number c. We also note that a positive-definite endomorphism must be monic since if α(v) = 0V implies that α(v), v = 0 and so v = 0V . Therefore every positivedefinite endomorphism of a finitely-generated inner product space is in fact an automorphism. Positive definite endomorphisms have important applications in optimization and linear programming. Note that if α is positive definite and if 0V = v ∈ V then 0 < α(v), v = α(v)·v cos(t), where t is the angle between α(v) and v, showing that 0 ≤ t < π2 . Example: Let V = Rn on which we have the dot product defined, and let B be the canonical basis. An endomorphism α of V is positive definite if and only if A = ΦBB (α) is a symmetric matrix satisfying the condition that v T Av > 0 for all nonzero vectors v ∈ V. Such matrices have nice properties. For example, it can be shown that if A is of this


357

form then the Gauss-Seidel method applied to an equation AX = w will converge to the unique solution v, for any initial guess v0 chosen. Example: Even if σ 0 = α ∈ End(V ) is selfadjoint, it may be the case that neither α nor −α is positive definite. For example, if V = R2 and ! ! a −a if α ∈ End(V ) is defined by α : → , then b b α

1 0

! ·

1 0

!

= −1 = (−α)

0 1

! ·

0 1

! .

Let V an inner product space. If α, β ∈ End(V ) are selfadjoint, then α − β is also selfadjoint. We will write α > β whenever α − β is positive definite. Thus, α is positive definite if and only if α > σ 0 . We will write α ≥ β if and only if α > β or α = β. We claim that this is a partial-order relation on the set of all selfadjoint endomorphisms of V. Indeed, it is sure that α ≥ α for all such endomorphisms α. Suppose that α1 , α2 , and α3 are selfadjoint endomorphisms of V satisfying α1 ≥ α2 ≥ α3 . If α1 = α2 or α2 = α3 then it is clear that α1 ≥ α3 . Let us therefore assume that α1 > α2 > α3 . Then for all v ∈ V we see that (α1 − α3 )(v), v

= α1 (v) − α2 (v) + α2 (v) − α3 (v), v = α1 (v) − α2 (v), v + α2 (v) − α3 (v), v > 0

and so α1 > α3 . Finally, assume that α1 ≥ α2 and α2 ≥ α1 but α1 = α2 . Then α1 > α2 > α1 and so, as we have seen, α1 > α1 , which is a contradiction. Thus we have a partial order on the set of all selfadjoint endomorphisms of V , called the Loewner2 partial order. (17.8) Proposition: Let V be an inner product space and let α ∈ End(V ) be an endomorphism for which α∗ exists. Then α is positive definite if and only if the function µ : (v, w) → α(v), w from V × V to the field of scalars is also an inner product.

2 Karl Loewner was a Czech mathematician who emigrated to the United States in 1933. His research concentrated in complex function theory and spaces of functions.

358


Proof: First, let us assume that α is a positive-definite endomorphism of V. If v1 , v2 , w ∈ V then µ(v1 + v2 , w) = α(v1 + v2 ), w = α(v1 ), w + α(v2 ), w = µ(v1 , w) + µ(v2 , w) and, similarly, we show that µ(cv, w) = cµ(v, w) for all scalars c. We also see that µ(v, w) = α(v), w = v, α∗ (w) = v, α(w) = α(w), v = µ(w, v). If 0V = v ∈ V then, by the assumption of positive definiteness, we see that µ(v, v) = α(v), v is a positive real number, and it is clear that µ(0V , 0V ) = 0. Thus µ is an inner product on V. Conversely, assume that µ is an inner product on V. Then for all v, w ∈ V we have v, α∗ (w) = α(v), w = µ(v, w) = µ(w, v) = α(w), v = v, α(w) and so α(w) = α∗ (w) for all w ∈ V, proving that α is selfadjoint. Moreover, for all v ∈ V we have α(v), v = µ(v, v) for all 0V = v ∈ V and so α is positive definite. (17.9) Proposition: Let V be an inner product space, with given inner product (v, w) → v, w , and let µ be another inner product defined on V. Then there exists a unique positivedefinite endomorphism α of V satisfying the condition that µ(v, w) = α(v), w for all v, w ∈ V. Proof: Fix a vector w ∈ V. The function v → µ(v, w) belongs to D(V ) and so there exists a unique vector yw ∈ V satisfying µ(v, w) = v, yw for all v ∈ V. Define a function α : V → V by α : w → yw . Then α(v), w = w, α(v) = µ(w, v) = µ(v, w) for all v, w ∈ V. We claim that α ∈ End(V ). Indeed, if w1 , w2 ∈ V then for all y ∈ V we have α(w1 + w2 ), y

= µ(w1 + w2 , y) = µ(w1 , y) + µ(w2 , y) = α(w1 ), y + α(w2 ), y = α(w1 ) + α(w2 ), y

and so α(w1 + w2 ) = α(w1 ) + α(w2 ). Similarly we can show that α(cw) = cα(w) for all w ∈ V and all scalars c. Thus we see that α is indeed an endomorphism of V satisfying the condition µ(v, w) = α(v), w for all v, w ∈ V, and so it is positive definite. Finally, α has to be unique since if µ(v, w) = β(v), w for all v, w ∈ V, then (α − β)(v), w = α(v) − β(v), w = α(v), w − β(v), w = 0 for all v, w ∈ V, which implies that (α − β)(v) = 0V for all v ∈ V, showing that α = β. (17.10) Proposition: Let V be a finitely-generated inner product space and let α ∈ End(V ). Then α is positive definite if and only if there exists an automorphism β of V satisfying α = β ∗ β. Proof: Assume that there exists an automorphism β of V satisfying α = β ∗ β. Then, as previously noted, α is selfadjoint. Moreover, for all 0V = v ∈ V we have α(v), v = β ∗ β(v), v = β(v), β ∗∗ (v) =


359

β(v), β(v) > 0 since β is an automorphism and hence β(v) = 0V . Therefore α is positive definite. Conversely, assume that α is a positive-definite endomorphism of V. Then the function µ : (v, w) → α(v), w is an inner product on V. Let {v1 , . . . , vn } be a basis for V which is orthonormal with respect to the original inner product on V and let {w1 , . . . , wn } be a basis for V which is orthonormal with respect to µ. By Proposition 6.2, we know that there exists a unique endomorphism β of V satisfying β(wi ) = vi for all 1 ≤ i ≤ n. Then β is an epimorphism since its image contains a basis for V and so, since V is nfinitelygenerated,it is an automorphism of V. Therefore, if v = i=1 ai wi n and w = j=1 bj wj are vectors in V we see that α(v), w = µ(v, w) = n n n n n = i=1 j=1 ai bj µ(wi , wj ) = i=1 ai bi and a w , b w µ i i j j i=1 j=1 D C n n = b w similarly β ∗ β(v), w = β(v), β(w) = β ( i=1 ai wi ) , β j j j=1 n n n ∗ i=1 j=1 ai bj wi , wj = i=1 ai bi , and so we see that β β(v), w = α(v), w for all v, w ∈ V, which shows that α = β ∗ β. Example: In order for an endomorphism to be positive definite, it is not enough for it to be represented by a matrix all of the entries of which are positive real numbers. For example, if V = R2 with the dot product, and if α is the endomorphism of V represented with respect to the ! ! ! 2 2 −1 −1 canonical basis by the matrix , then α · = 2 1 1 1 ! ! 0 −1 · = −1, so α is not positive definite. −1 1 From Proposition 17.10 we know that if A = [aij ] ∈ Mn×n (C) is a matrix representing a positive-definite endomorphism of Cn , namely if it is a Hermitian matrix satisfying the condition that v · Av > 0 for all nonzero vectors v ∈ Cn , then there exists a nonsingular matrix B such that A = B H B. Indeed, we can choose B to be upper triangular, so that it is a form of LU-decomposition, though it takes only half as many arithmetic operations to perform. This decomposition is known as a Cholesky3

3

Major Andr´ e-Louis Cholesky was a cartographer in the French army, who used this method in connection with the mapping of the island of Crete before World War I. It had previously been used by other cartographers, including Myrick H. Doolittle, of the computing division of the US Coast and Geodetic Survey, in 1878.

360


decomposition of A. This decomposition need not be unique. Cholesky decompositions are widely used in building economic and financial models. Because of this wide usage, there are many algorithms available to efficiently calculate Cholesky decompositions of general matrices or of matrices in special forms. Indeed, one of the computational advantages of the Cholesky decomposition is that it is numerically stable, even with no pivoting. The following algorithm calculates a Cholesky decomposition for real symmetric matrices. For k = 1, . . . , n perform the following steps: * + i−1 aik − j=1 bji bjk ; (1) For each 1 ≤ i < k define bik = b−1 ii 7 k−1 (2) Set bkk = akk − j=1 b2jk ; (3) For each k < i ≤ n set bik = 0. Note that if the matrix A did not satisfy v · Av > 0 for all nonzero vectors v, the algorithm would hang up at some stage, trying to take the square root of a negative number. Indeed, attempting a Cholesky decomposition is often used as a test to see whether a given matrix represents a positive-definite endomorphism or not. 

5 Example: Let A =  2 3

2 1 1

 3 1  ∈ M3×3 (R). This is a symmet4

ric matrix satisfying the condition that v · Av > 0 for all nonzero vectors v ∈ R3 and having a Cholesky decomposition B T B, where B = √ √   √ 5 5 2√5 3√5 1 0 5 −√5  . 5 0 0 5 2 Notice that the Proposition 17.10 extends our ongoing analogy between the operation ∗ and the conjugate operation on C, just as the notion of “positive definite” is the analog of positivity of complex numbers: a complex number z is (real and) positive if and only if there exists a complex number y such that z = yy. (17.11) Proposition: Let V be an inner product space. If α ∈ End(V ) is positive definite, then every eigenvalue of α is a positive real number. The converse holds if α is orthogonally diagonalizable.


361

Proof: Assume that α is positive define. By Proposition 17.4, the eigenvalues of α are real numbers. If c ∈ spec(α) is an eigenvalue of α associated with an eigenvector v, then 0 < α(v), v = cv, v = c v, v and so c > 0, since we know that v, v > 0. Conversely, assume that every eigenvalue of α is positive and that there existsan orthonormal n basis B of V composed of eigenvectors of α. Let v = i=1 ai vi , where {v1 , . . . , vn } ⊆ B. For each 1 ≤ i ≤ n, let ci be an eigenvalue of α associated with vi . We can assume that the vi are arranged in such a manner that 0 < c1 ≤ c2 ≤ . . . ≤ cn . Then 8 n 9 n n n α(v), v = α(ai vi ), aj vj = ai aj ci vi , vj i=1

=

j=1

n n

i=1 j=1

ci ai aj vi , vj =

i=1 j=1

n

ci |ai |2 ≥ c1

i=1

n

|ai |2 > 0

i=1

and so α is positive definite.

. From Propositions 17.11 and 17.7, we see that if V is an finitelygenerated inner product space over R or C and if α ∈ End(V ) is positive definite, then there exists a basis of V relative to which α is represented by a diagonal matrix in which the entries of the diagonal are positive real numbers. Such a matrix is, of course, nonsingular. (17.12) Proposition: Let V and W be inner-product spaces √ finitely-generated over R and let α ∈ Hom(V, W ). Then α = c, where c is the largest eigenvalue of α∗ α ∈ End(V ), and where α is the norm induced by the respective inner products on V and W. Proof: If c is an eigenvalue of β = α∗ α then there exists a nonzero 2 vector v such that β(v) = cv and so c v = v, cv = v, α∗ α(v) = α(v), α(v) ≥ 0, and so c ≥ 0. By Proposition 17.7, we know that there exists a basis {v1 , . . . , vn } of V composed of orthonormal eigenvectors of β. For each 1 ≤ i ≤ n, let ci be an eigenvalue of β associated withvi . After renumbering, we can assume that 0 ≤ c1 ≤ . . . ≤ cn . If n v = i=1 ai vi ∈ V, then 2

α(v)

=

=

v, β(v) = v, α∗ α(v) = n i=1

" ci a2i ≤ cn

n i=1

# a2i

n n

aj ci ai vj , vi

j=1 i=1 2

= cn v

362

17. Selfadjoint Endomorphisms 2

2

and so α(v) / v ≤ cn . Therefore, by definition of the induced norm, √ 2 2 α ≤ cn . But one easily sees that α(vn ) / vn = cn and so √ cn ≤ α , proving equality. Example: Let α : R3 → R2 be the linear transformation defined ! 1 −2 1 by α : v → Av, where A = . Then α∗ α is the 3 0 −1   10 −2 −2 4 −2  v. The eigenvalues endomorphism of R3 given by v →  −2 −2 −2 2 √ √ √ of this endomorphism are 0 ≤ 8−2 2 ≤ 8+2 2 and so α = 8 + 2 2, which is approximately equal to 3.291. Let V and W be inner product spaces. A linear transformation α : V → W preserves inner products if and only if v1 , v2 = α(v1 ), α(v2 ) for all v1 , v2 ∈ V. Notice that any linear transformation which preserves inner products also preserves distances: v1 − v2 = α(v1 − v2 ) = α(v1 ) − α(v2 ) for all v1 , v2 ∈ V. Also, as a direct consequence of the definition, such a linear transformation preserves the angles between vectors. Conversely, we have already noted that from the norm defined by an inner product we can recover the inner product itself, so that any linear transformation α : V → W satisfying v1 − v2 = α(v1 ) − α(v2 ) for all v1 , v2 also preserves inner products. Such a linear transformation is called an isometry. We also note that if α is an endomorphism of an inner product space V which is an isometry, and if c is an eigenvalue of α with associated 2 2 2 eigenvector v, then v = cv = |c|2 v and so |c| = 1. Thus, if V is an inner product space over C and if α ∈ End(V ) is an isometry, then the eigenvalues of α lie on the unit circle {z ∈ C | |z| = 1}. Example: Let V be an inner product space over R and let 0V = y ∈ V. This vector y defines an endomorphism αy of V by setting αy : v → −v + 2

v, y y. y, y

This endomorphism is an isometry which satisfies α2y = σ 1 , and y is a fixed point of αy . (17.13) Proposition: Let V and W be finitely-generated inner product spaces and having equal dimensions. Then the following conditions on a linear transformation α : V → W are equivalent: (1) α is an isometry; (2) α is an isomorphism which is an isometry;


(3) If {v1 , . . . , vn } is an orthonormal basis of V {α(v1 ), . . . , α(vn )} is an orthonormal basis of W.

363

then the set

Proof: (1) ⇒ (2): If 0V = v ∈ V then v, v = α(v), α(v) and so α(v) = 0W . Thus we see that ker(α) = {0V } and so α is an isomorphism, since V and W have the same finite dimension. (2) ⇒ (3): If {v1 , . . . , vn } is an orthonormal basis of V then, since α is an isomorphism, we see that {α(v1 ), . . . , α(vn )} is a basis for W. Moreover, for all 1 ≤ i, j ≤ n we know that

1 when i = j α(vi ), α(vj ) = vi , vj = 0 otherwise and so this basis is orthonormal. ⇒ (1): Let {v 1n, . . . , vn } be an orthonormal n basis of V. If v = (3) n a v and y = b v , then v, y = i=1 i i j=1 j j i=1 ai bi . Moreover, α(v), α(y) =

9 #  n 8 " n ai vi , α  bj vj  α i=1

=

n n

j=1

ai bj α(vi ), α(vj ) =

i=1 j=1

and this proves (1).

n

ai bi = v, y

i=1

In particular, if V and W are finitely-generated inner product spaces having equal dimensions, then every isometry Eα : V → W is an Fisomorphism. If w1 ,Fw2 ∈ W, then w1 , w2 = αα−1 (w1 ), αα−1 (w2 ) = E −1 α (w1 ), α−1 (w2 ) and so we see that α−1 is also an isometry. Moreover, there is always at least one isometry α from V to W. Just pick orthonormal bases{v1 , . . . , vn } for V and {w1 , . . . , wn } for W and n n define α by α : i=1 ai vi → i=1 ai wi . Example: Let W be the set of all matrices A ∈ M3×3 (R) satisfying AT = −A, which is a subspace of M3×3 (R) of dimension 3. Define an inner product on W as follows: if A, B ∈ W then A, B = 1 T 3 2 tr(AB ). Let V = R , which is an inner product space with respect to the dot product. Define a linear transformation α : V → W by       a 0 −c b 0 −c b 0 −a  . If A =  c 0 −a  and setting α :  b  →  c c −b a 0 −b a 0     cf + be −bd −dc 0 −f e  ea cf + ad ec 0 −d  then AB T =  B =  f −af fb be + ad −e d 0

364




   a d and so we can check that A, B =  b  ·  e  and thus α is an c f isometry and hence is an isomorphism. Example: Proposition 17.13 is no longer true if we remove the condition that the spaces are finitely generated. Indeed, let V = C(0, 1), on which 41 we have the inner product µ(f, g) = 0 f (x)g(x)x2 dx, and let W be the 41 same space on which we have the inner product f, g = 0 f (x)g(x)dx. Let α : V → W be the linear transformation defined by α : f (x) → xf (x). Then µ(f, g) = α(f ), α(g) and so α is an isometry. But α is not an isomorphism since the function x → x2 + 1 does not belong to the image of α. Let us now return to the case of inner product spaces the dimensions of which are not necessarily equal. (17.14) Proposition: Let V and W be inner product spaces finitely-generated over R and let α ∈ Hom(V, W ). Then α is an isometry if and only if α∗ α = σ 1 ∈ End(V ). Proof: By Proposition 16.14, α∗ exists. If α∗ α = σ 1 ∈ End(V ), and if v1 , v2 ∈ V then v1 − v2

2

=

v1 − v2 , v1 − v2 = v1 − v2 , α∗ α(v1 − v2 ) 2

= α(v1 − v2 ), α(v1 − v2 ) = α(v1 ) − α(v2 )

and so v1 − v2 = α(v1 ) − α(v2 ) , proving that α is an isometry. Conversely, if α is an isometry and if v1 , v2 ∈ V then α∗ α(v1 ), v2 = α(v1 ), α(v2 ) = v1 , v2 . Therefore, by Proposition 16.13, we see that α∗ α(v1 ) = v1 for all v1 ∈ V, proving that α∗ α = σ 1 ∈ End(V ).

Exercises Exercise Let V = C[X]F and E945 ∞define an inner product on V by ∞ ∞ i i = i=0 ai bi . Let α be the endomorphism setting i=0 ai X , i=0 bi X of V defined by α : p(X) → (X + 1)p(X). Calculate α∗ , or show that it does not exist.


365

Exercise Let V = C[X]F and E946 ∞define an inner product on V by ∞ ∞ i i = a X , b X setting i i i=0 i=0 i=0 ai bi . Let β be the endomorphism of V defined by β : p(X) → p(X + 1). Calculate β ∗ , or show that it does not exist. Exercise 947 Let p > 1 be an integer, let G = Z/(p), and let V = CG , which is an inner product space over C with inner product defined by f, g = n∈G f (n)g(n). Let α be the endomorphism of V defined by α(f ) : n → f (n + 1) + f (n − 1). Is α selfadjoint? Exercise 948 Let V be a vector space over R. A nonempty subset K of V is convex if and only if cv + (1 − c)w ∈ K whenever v, w ∈ K and 0 ≤ c ≤ 1. Is the set of all selfadjoint endomorphisms of an inner product space Y over R necessarily a convex subset of the vector space End(Y )? Exercise 949 Let V be an inner product space and let α be an endomorphism of V. Is the endomorphism α∗ α − σ 1 of V selfadjoint? Exercise 950 Let n be a positive integer and let V be the space of all polynomial functions in RR4 of degree at most n. Define an inner product 1 on V by setting f, g = −1 f (t)g(t)dt. Let α ∈ End(V ) be defined by α(f ) : x → 1 − x2 f (x) − 2xf (x). Show that α is self-adjoint. Exercise 951 Let V be an inner product space finitely generated over C and let α be an endomorphism of V satisfying αα∗ = α2 . Show that α is selfadjoint. Exercise 952 Let V be an inner product space finitely generated over C and let α and β be selfadjoint endomorphisms of V satisfying the condition that αβ is a projection. Is βα necessarily also a projection? Exercise 953 Give an example of nonzero Hermitian matrices A and B satisfying AB = O = BA, or show no such matrices exist. Exercise 954 Let A ∈ M2×2 (C) be Hermitian. Find real numbers w, x, y, and z satisfying |A| = w2 − x2 − y 2 − z 2 . Exercise 955 Let n be a positive integer and let A ∈ Mn×n (C). Show that A is a Hermitian matrix if and only if the matrix B = iA satisfies B = −B H . Exercise 956 Let O = A ∈ M3×3 (C) be a Hermitian matrix. Ak = O for all positive integers k.  a Exercise 957 Find complex numbers a and b such that  0 i M3×3 (C) is a Hermitian matrix.

Show that  0 b 2a a  ∈ 1 a

366


Exercise 958 A matrix A ∈ Mn×n (C) is anti-Hermitian if and only if AH = −A. Show that A is anti-Hermitian if and only if iA is Hermitian. Exercise 959 If matrices A, B ∈ Mn×n (C) are anti-Hermitian, show that the Lie product of A and B is also anti-Hermitian. Exercise 960 Let n be a positive integer and let A ∈ Mn×n (C). Show that every eigenvalue of AH A is a positive real number. Exercise 961 Let V be an inner product space and let α ∈ End(V ) be selfadjoint. Show that ker(α) = ker(αh ) for all h ≥ 1. Exercise 962 Let V be a nontrivial finitely-generated inner product space and let α ∈ End(V ) be orthogonally diagonalizable and satisfy the condition that each of its eigenvalues is real. Is α necessarily selfadjoint? Exercise 963 Let V = R2 , endowed with the dot product. Is the endo! ! a a+b morphism α of V defined by α : → positive definite? b a+b Exercise 964 Let α ∈ End(R3 ) be represented with respect to the canoni  1 2 3 cal basis by the matrix  2 a 4  . For which values of a is α positive 3 4 5 definite? Exercise 965 For each complex number z, let αz be the endomorphism   1 1 −1 z . of C3 represented with respect to the canonical basis by  1 1 1 −1 z Does there exist a z for which this endomorphism is positive definite? Exercise 966 Let V be an inner product space and let α ∈ End(V ) be positive definite. Is α2 necessarily positive definite? Exercise 967 Let α be a positive definite automorphism of an inner product space V. Is α−1 necessarily positive definite? Exercise 968 Let k and n be positive integers. A symmetric matrix ! −B AT in Mk+n,k+n (R) is quasidefinite when it is of the form A C where B is a matrix representing a positive-definite endomorphism of Rk with respect to the canonical basis, and C is a matrix representing a positive-definite endomorphism of Rn with respect to the canonical basis. Show that a quasidefinite matrix is nonsingular, and that its inverse is again quasidefinite.


367

Exercise 969 Let V = R2 together with the dot product. Find positivedefinite endomorphisms α and β of V satisfying the condition that their Jordan product is not positive definite. Exercise 970 Let V be an inner product space over R and let α ∈ End(V ). Show that α is positive definite if and only if α + α∗ is positive definite. Exercise 971 Let V be an inner product space finitely generated over C and let α and β be positive-definite endomorphisms of V satisfying αβ = σ 0 . Is it necessarily true that α = σ 0 or β = σ 0 ?    a        b   Exercise 972 Let V =  a, b, c ∈ R and let W = R3 , both  b       c of which together with the dot product, are inner product spaces of dimension 3 over R. Find an isomorphism α : V → W which is also an isometry. Exercise 973 Let V be an inner product space and let α be an endomorphism of V which is an isometry. Does α also preserves angles between vectors? Exercise 974 Let α be a positive-definite endomorphism of a finitedimensional inner product space V represented with respect to some fixed n aii . basis by an n × n matrix A = [aij ]. Show that |A| ≤ i=1

Exercise 975 Let n be a positive integer and let α be a positive-definite endomorphism of Cn represented with respect to the canonical basis by the matrix A = [aij ] ∈ Mn×n (C). Show that aii is a positive real number for all 1 ≤ i ≤ n. Exercise 976 Let α : R3 → R2 be the linear transformation defined by   ! a b − 2c α :  b  → . Calculate spec(αα∗ ) and spec(α∗ α). a+c c Exercise 977 Let n be a positive integer and let V = Rn , on which we have defined the dot product. Let α be a positive-definite endomorphism of V represented with respect to the canonical basis by the matrix A = [aij ] ∈ Mn×n (R). Show that |A| > 0. Is it necessarily true that tr(A) > 0? Exercise 978 Let V = C2 . Find endomorphisms α, β ∈ End(V ) satisfying α > β (in the sense of Loewner) but not α2 > β 2 .

368


Exercise 979 Let V be an inner product space and let α, β ∈ End(V ) be positive definite. Is it necessarily true that α + β > β? Exercise 980 Let V and W be inner product spaces finitely generated over C. Let α ∈ Hom(V, W ), θ ∈ Aut(V ), and ϕ ∈ Aut(W ), where the automorphisms θ and ϕ are positive definite. Show that the automorphism θ − α∗ ϕα of V is positive definite if and only if the automorphism ϕ − αθα∗ of W is positive definite. Exercise 981 Let V be the vector space of all infinitely-differential func4π tions in RR , on which we define the inner product f, g = 0 f (x)g(x)dx. Let W be the subspace of all functions f ∈ V satisfying f (0) = f (π) = 0. Show that the endomorphism of W defined by f → f is selfadjoint. Exercise 982 Let V be a finitely-generated inner product space and let α ∈ End(V ) be selfadjoint. Show that α(v) ≤ v for all v ∈ V. Exercise 983 Let V be an inner product space finitely generated over R of dimension greater than 1, and let α be a selfadjoint endomorphism 2 of V. Show that there are eigenvalues c < d of α satisfying c v ≤ 2 α(v), v ≤ d v for all v ∈ V. Exercise 984 Let V be an inner product space finitely generated over and let α, β ∈ End(V ) be selfadjoint. Assume that the eigenvalues of all lie in the interval [a, b] on the real line and that the eigenvalues of all lie in the interval [c, d] on the real line. Show that the eigenvalues α + β all lie in the interval [a + c, b + d] of the real line.

R α β of

Exercise 985 Let V be an inner product space finitely generated over C and α be a positive-definite selfadjoint automorphism of V. Show that F E let −1 (α + α )(v), v ≥ 2 v, v for all v ∈ V. Exercise 986 Let V be an inner product space finitely generated over R and E −1let α Fbe a positive-definite selfadjoint automorphism of V. Show that α (v), v = max{2 v, w − α(w), w | w ∈ W } for all v ∈ V. Exercise 987 Let V be a vector space finitely-generated over R and let α ∈ End(V ) be selfadjoint. Show that at least one of the values ± α is an eigenvalue of α and any eigenvalue c of α satisfies − α ≤ c ≤ α . ! a b ∈ M2×2 (C) be Hermitian and let r ≥ s Exercise 988 Let A = b c be the (necessarily real) eigenvectors of A. Show that |b| ≤ 12 (r − s).

18 Unitary and Normal endomorphisms

Let V be an inner product space. An automorphism of V which is an isometry is called a unitary automorphism. It is easy to see that if α and β are unitary automorphisms of V then αβ and α−1 are also unitary automorphisms of V. It is also clear that σ 1 is unitary. Therefore, the set of all unitary automorphisms of V is a group of automorphisms. (18.1) Proposition: Let V be an inner product space and let α ∈ Aut(V ) have an adjoint. Then α is unitary if and only if α∗ = α−1 . F E F E Proof: If α is unitary then α(v), w = α(v), αα−1 (w) = v, α−1 (w) for all v, w ∈ V and so α∗ = α−1 . Conversely, if α∗ = α−1 then α(v), α(w) = v, α∗ α(w) = v, w for all v, w ∈ V and so α is unitary. As a direct consequence of Proposition 17.13, we see that if V is an inner product space finitely generated over its field of scalars then for α ∈ End(V ) the following conditions are equivalent: (1) α is an isometry; (2) α is unitary; (3) α maps an orthonormal basis of V to an orthonormal basis of V. If V is an inner product space finitely generated over its field of scalars F, and if α is a unitary automorphism of V represented by a matrix 369

370

18. Unitary and Normal endomorphisms

A = [aij ] ∈ Mn×n (F ) with respect to a given orthonormal basis. Then we see that A−1 = AH ∈ Mn×n (F ). A matrix of this form over F is called a unitary matrix. If A is a unitary matrix then so is A−1 since (A−1 )H = (AH )−1 . Also, if A and B are unitary matrices then (AB)−1 = B −1 A−1 = B H AH = (AB)H so AB is also unitary. The ! −1 1 converse is false. For example, the matrix A = ∈ M2×2 (R) 0 1 is not unitary, but A2 = I is. Thus we see that the set of unitary matrices in Mn×n (F ) define a group of automorphisms of F n and so an equivalence relation ∼ defined by the condition that A ∼ B if and only if there exists a unitary matrix P such that A = P −1 BP. Matrices equivalent in this sense are unitarily similar. As an immediate consequence of the definition, we see that A is unitary if and only if the set of columns [resp. rows] of A is an orthonormal basis of F n [resp. M1×n (F )] endowed with the dot product.

(18.2) Proposition: Let n be a positive integer and let A = [aij ] unitarily-similar matrices in Mn×n (C). Then and B = [bij ] be n n n n 2 2 |a | = |b | . ij ij i=1 j=1 i=1 j=1 n n 2 H Proof: We note that i=1 j=1 |aij | = tr(A A). If P is a unitary matrix satisfying B = P −1 AP then tr(B H B) = tr(P −1 AH P P −1 AP ) = tr(P −1 AH AP ) = tr(AH AP −1 P ) = tr(AH A), and we are done.

Example: If c, d ∈ C satisfy the condition that |c|2 + |d|2 = 1, then ! c d the matrix ∈ M2×2 (C) is unitary. A matrix of this form is −d c known as a Givens1 rotation matrix. More generally, if n > 3 then a matrix A = [aij ] ∈ Mn×n (C) is a Givens rotation matrix if and only if there exist integers 1 ≤ h < k ≤ n and nonzero complex numbers c and

1 James Wallace Givens, a former assistant to Von Neumann, is considered to be one of the fathers of 20th-century American numerical analysis, who made major contributions to numerical matrix computation.


371

d satisfying |c|2 + |d|2 = 1 such that  c if i = j ∈ {h, k}     1 if i = j ∈ / {h, k}  d if i = h and j = k . aij =    −d if i = k and j = h   0 otherwise These matrices play important roles in numerical algorithms. ! 1−i 1+i ∈ M2×2 (C) is uni1+i 1−i tary. This matrix has important applications in the modeling of quantum ! √ 0 1 computing, where it is often denoted by N OT , since A2 = 1 0 represents the negation operator in this context. Example: The matrix A =

1 2

√

! 1 + b2 √ bi ∈ Example: It is easy to show that Ab = 1 + b2 −bi M2×2 (C) satisfies Ab ATb = I for any real number b, but, except for the case of b = 0, it is not unitary. Unitarily-similar matrices are surely similar, but the converse is not true. Example: The matrices

3 −2

1 0

! and

1 1 0 2

! in M2×2 (R) are

similar but not unitarily similar, as we can see from Proposition 18.2. (18.3) Proposition (Schur’s Theorem2 ): If n is a positive integer, then every matrix in Mn×n (C) is unitarily similar to an upper-triangular matrix. Proof: We will proceed by induction on n. For n = 1, the result is trivial since every 1 × 1 matrix is upper triangular. Assume now that n > 1 and that the result has been established for M(n−1)×(n−1) (C). Let A = [aij ] ∈ Mn×n (C). Since we are working over C, we know that the

2

Issai Schur was a 20th-century German mathematician who is known primarily for his work in group theory.

372


characteristic polynomial of A is completely reducible, and so A has an eigenvalue, call it c1 . Corresponding to that eigenvalue, we have a normal   d1   eigenvector v1 =  ...  in which we can assume that d1 ∈ R. We now dn are able to construct a basis {v1 , . . . , vn } for Cn to which we can apply the Gram-Schmidt procedure, and thus assume that it is in fact an orthonormal basis (the vector v1 doesn’t change, since it was assumed to be normal to begin with). The matrix P1 , the columns of which are these vectors, is therefore unitary. Now set A1 = P1−1 AP1 . It is easy to see that the first   c1  0    column of A1 is of the form  .  so we can write A1 in block form as  ..  0 ! c1 x , where A2 ∈ M(n−1)×(n−1) (C). By the induction hypothesis, O A2 there is a unitary matrix Q ∈ M(n−1)×(n−1) (C) such!that Q−1 A2 Q is 1 O an upper-triangular matrix. Now set P2 = . Then P2 is a O Q ! c1 y is unitary matrix in Mn×n (C) and P2−1 P1−1 AP1 P2 = O Q−1 A2 Q an upper triangular matrix in Mn×n (C). Since P1 P2 is again unitary, we are done. If we are working over R, then a matrix A representing a unitary automorphism of Rn satisfies A−1 = AT . Such a matrix is called an orthogonal matrix. It is clear that the matrix I is orthogonal and that A−1 is orthogonal whenever A is orthogonal. If A and B are orthogonal matrices then (AB)−1 = B −1 A−1 = B T AT = (AB)T and so AB is also orthogonal. As an immediate consequence of the definition, we see that A is orthogonal if and only if the set of columns [resp. rows] of A is an orthonormal basis of Rn [resp. M1×n (R)] endowed with the dot product. It is also clear that A is orthogonal if and only if AT is orthogonal. Example: Permutation matrices, which we considered earlier, are clearly orthogonal. Example: The matrices

cos(t) sin(t) − sin(t) cos(t)

! and

cos(t) sin(t)

sin(t) − cos(t)

!

are orthogonal for every t ∈ R, and one can show that these are the only orthogonal matrices in M2×2 (R). Indeed, suppose that the matrix


a11 a21

a12 a22

373

! ∈ M2×2 (R) is orthogonal. Then a211 +a212 = 1 = a221 +a222 so

−1 ≤ a11 ≤ 1. Hence there exists a real number t such that a11 = cos(t). Then a212 = 1 − a211 = 1 − cos2 (t) = sin2 (t) and so a12 = ± sin(t). Also, a11 = cos(−t) and sin(−t) = − sin(t). Thus, replacing t by −t if necessary we can assume that a11 = cos(t) and a12 = sin(t). Similarly, there exists an angle s such that a22 = cos(s) and a21 = sin(s). Since 0 = a11 a21 + a12 a22 = cos(t) sin(s) + sin(t) cos(s) = sin(t + s), we see that t + s = 0 or t + s = π. If t + s = 0, we obtain ! cos(t) sin(t) A= . − sin(t) cos(t) ! cos(t) sin(t) If t + s = π, then s = π − t and so A = since sin(t) − cos(t) sin(t) = sin(π − t) and − cos(t) = cos(π − t). One can also show that every orthogonal matrix in M3×3 (R) is similar   cos(t) − sin(t) 0 cos(t) 0  for some t ∈ R. to a matrix of the form  sin(t) 0 0 ±1 Example: Let √n be a positive √ integer. ! If 0 ≤ c ≤ 1 is a real number, c) I − 1 − c I ( √ √ ∈ M2n×2n (R) is orthogonal, the matrix 1−c I ( c) I where I denotes the identity matrix in Mn×n (R). Example: Let n be a positive integer and let V = Rn , on which we have defined the dot product. If v ∈ V is a normal vector, then the matrix A = I − 2(v ∧ v) is a Householder3 matrix. These matrices are clearly symmetric. Moreover, if A = I − 2(v ∧ v) then AT A = A2 = (I − 2[v ∧ v])2 = I − 4v(v T v)v T + 4v(v T v)v T = I and so A is orthogonal. Householder matrices have important uses in numerical analysis. We should also mention that if u = v are vectors

3 Alston Householder, a 20th-century American mathematician, was among the pioneer researchers of the numerical analysis of matrices using computers, who developed many of the basic algorithms used in this field.

374

18. Unitary and Normal endomorphisms −1

in V satisfying u = v , then the vector w = v − u (v − u) defines a Householder matrix A = I − 2(w ∧ w) satisfying Au = Av. Since a Householder matrix is totally determined by one vector, it is easy to store in a computer. One of the important uses of Householder matrices is to compute QR-decompositions of matrices in a manner far more stable numerically than via the use of the Gram-Schmidt method. The complex analog of Householder matrices are matrices of the form I − 2wwH , where w ∈ Cn . Such matrices are Hermitian and unitary and, too, have an important role in numerical computation. Example: A general method for the construction of orthogonal matrices, due to contemporary American mathematician George W. Soules, is given as follows: Let n > 1 be an integer and let w1 ∈ Rn be a normal vector all of the entries of which are all positive. Let 1 ≤ k < n ! v u , where u ∈ Rk and v ∈ Rn−k . Set a = and write w1 = v u ! au and w2 = . Then it is easy to see that w2 is normal and −a−1 v orthogonal to w1 . Moreover, by further partitioning the vectors au and −a−1 v, we can eventually construct a mutually-orthogonal normal vectors w1 , w2 , . . . , wn . The matrix with these vectors as columns is then orthogonal. Notice that if F is either R or C, and if A ∈ Mn×n (F ) is a unitary matrix the columns of which are v1 , . . . , vn , then the identity AAH = I implies that {v1 , . . . , vn } is an orthonormal set of vectors in F n , on which we have the dot product, and hence it is a basis for this space. Conversely, if {v1 , . . . , vn } is an orthonormal basis of F n then the matrix the columns of which are these vectors is unitary. Similarly, a matrix in Mn×n (R) is orthogonal if and only if the set of its columns forms an orthonormal basis for Rn with the dot product. Another way of putting this is that a matrix the columns of which are v1 , . . . , vn is orthogonal if and in Mn×n (R) n v ∧ vi = I. only if i i=1 (18.4) Proposition: Let V be an inner product space of finite dimension n over R. Let α be a unitary automorphism of V, which is represented by a matrix A ∈ Mn×n (R) with respect to a given orthonormal basis of V. Then |A| = ±1. Proof: We know that if α is represented by A = [aij ] with respect to the given basis, then α∗ is represented by AT . From Proposition 18.1, we deduce that AAT = I and so |A|2 = |A| · |AT | = |I| = 1, and so |A| = ±1.


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The orthogonal matrices in Mn×n (R) having determinant equal to 1 are known as the special orthogonal matrices, and the set of all such matrices is denoted by SO(n). This subset of Mn×n (R) is clearly closed under taking products as well as taking inverses, since if A ∈ SO(n) then |A−1 | = |AT | = |A| = 1. If A ∈ Mn×n (R) is a special orthogonal matrix, where n is an odd integer, then 1 ∈ spec(A). To see this, we note that |A − 1I| = |A − I| = |A − AAT | = |A| · |I − AT | = |I − AT | = |I − A| and, since n is odd, |I−A| = (−1)n |A−I|. Thus we must have |A−I| = 0, and so 1 ∈ spec(A). Example: We have already noted that the only orthogonal matrices in ! ! cos(t) sin(t) cos(t) sin(t) or M2×2 (R) are of the form − sin(t) cos(t) sin(t) − cos(t) for some t ∈ R. Matrices of the first type are special, whereas matrices of the second type are not. Let V be an inner product space. An endomorphism α ∈ End(V ) is normal if and only if α∗ exists and satisfies α∗ α = αα∗ . From this definition, it is clear that α is normal if and only if α∗ is normal. Clearly selfadjoint endomorphisms of V are normal, as are unitary automorphisms. Example: If a, b ∈ R satisfy b = 0 and a2 + b2 = 1, then the ! ! c ac + bd 2 automorphism α of R defined by → is normal but d ad − bc neither unitary nor selfadjoint. Example: If 0 = a, b ∈ R then the automorphism α of C2 defined ! ! c c + id by → is normal but neither unitary and nor selfadjoint. d c − id (18.5) Proposition: Let V be an inner product space. An endomorphism α ∈ End(V ) for which α∗ exists is normal if and only if α(v) = α∗ (v) for all v ∈ V. 2

Proof: If α is normal and v ∈ V, then α(v) = α(v), α(v) = 2 v, α∗ α(v) = v, αα∗ (v) = v, α∗∗ α∗ (v) = α∗ (v), α∗ (v) = α∗ (v) ∗ and so α(v) = α (v) . Conversely, assume that this condition holds. Then for each v ∈ V we have (αα∗ − α∗ α)(v), v = αα∗ (v), v − α∗ α(v), v = α∗ (v), α∗ (v) − α(v), α(v) = 0.

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But αα∗ − α∗ α is selfadjoint and so, by Proposition 17.3 we see that αα∗ − α∗ α = σ 0 , and so αα∗ = α∗ α. We now take a short look at the extensive theory of eigenvalues of normal endomorphisms of inner product spaces. We will restrict our attention to finite-dimensional spaces, since the theory for infinite-dimensional spaces requires additional topological assumptions.4 (18.6) Proposition: Let V be an inner product space and let α ∈ End(V ) be normal. Then every eigenvector of α is also an eigenvector of α∗ and if c is an eigenvalue of α then c is an eigenvalue of α∗ . Proof: If v ∈ V then, as we have noted, α(v) = α∗ (v) . For a scalar c, we see that (α − cσ 1 )∗ (α − cσ 1 )

= (α∗ − cσ 1 )(α − cσ 1 ) = (α − cσ 1 )(α∗ − cσ 1 ) = (α − cσ 1 )(α − cσ 1 )∗

and so α−cσ 1 is also normal. Thus, (α − cσ 1 )(v) = (α∗ − cσ 1 )(v) for v ∈ V and so, in particular, we see that v ∈ ker(α − cσ 1 ) if and only if v ∈ ker(α∗ − cσ 1 ). In other words, v is an eigenvector of α associated with the eigenvalue c if and only if it is an eigenvector of α∗ associated with the eigenvalue c. Since α∗∗ = α for any endomorphism α of V , we see from Proposition 18.6 that if α is normal then a scalar c is an eigenvalue of α if and only if c is an eigenvalue of α∗ . Another interesting consequence of Proposition 18.6 is the following: let V be a finitely-generated inner product space and let α ∈ Aut(V ) be unitary. Then α is surely normal. If c ∈ spec(α) then c = 0 since α is an automorphism. If v is an eigenvector associated with c then v = (α∗ α)(v) = α∗ (cv) = cα∗ (v) and so α∗ (v) = c−1 v. This shows that c−1 is an eigenvalue of α∗ and hence, by Proposition 18.6, c−1 ∈ spec(α).

4 The study of eigenvalues of normal and selfadjoint endomorphisms of inner product spaces was developed simultaneously by the American mathematician Marshall Stone and by John von Neumann, inspired by problems in quantum theory.


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Example: In Proposition 17.5 we saw that if α is a selfadjoint endomorphism of an inner product space V finitely generated over R, then spec(α) = ∅. This is not necessarily true for normal endomorphisms of inner product spaces which are not selfadjoint. For example, let V = R2 together with the dot product, and if α ∈ End(V ) is defined by ! ! a −b α: → , then we have already seen that spec(α) = ∅. One b a can easily check that α is normal but not selfadjoint. (18.7) Proposition: Let V be an inner product space finitely generated over C and let α ∈ End(V ). Then α is normal if and only if it is orthogonally diagonalizable.

Proof: Assume that α is normal. We will proceed by induction on n = dim(V ). First assume that n = 1. Since we are working over C, we know that spec(α) = ∅ and so there exists a normal eigenvector v1 of α. Then V = Cv1 and we are done. Now assume that n > 1 and that the result has been proven for subspaces of dimension n − 1. Again, there exists a normal eigenvector v1 of α. Set W = Cv1 . The subspace W of V is invariant under α, and so, by Proposition 18.6, it is also invariant under α∗ . Therefore W ⊥ is invariant under α∗∗ = α. The restriction of α to W ⊥ is a normal endomorphism, the adjoint of which is the restriction of α∗ to W ⊥ . By induction, we know that there exists an orthonormal basis {v2 , . . . , vn } composed of eigenvectors of α, and so {v1 , . . . , vn } is the basis of V we are seeking. Conversely, assume that there exists an orthonormal basis of B = {v1 , . . . , vn } composed of eigenvectors of α. Then ΦBB (α) = [aij ] is a diagonal matrix satisfying the condition that each aii is an eigenvalue of α. Moreover, ΦBB (α∗ ) = ΦBB (α)H and this too is a diagonal matrix. Since diagonal matrices commute, we see that αα∗ = α∗ α and so α is normal. Note that Proposition 18.7 does not imply that if V is an inner product space finitely generated over C and if α ∈ End(V ) is normal, then every basis B of V composed of eigenvectors of α is necessarily orthonormal or that its elements are even necessarily mutually orthogonal, merely that one such basis exists. Example: Let α be the endomorphism of C4 represented with respect   1 2 0 0  −2 1 0 0   to the canonical basis by the matrix A =   0 0 3 −1  . One easily 0 0 1 3

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checks that AAH = AH A and so α is a normal automorphism of C4 . The characteristic polynomial of A is X 4 − 8X 3 + 27X 3 − 50X + 50 = (X 2 − 6X + 10)(X 2 − 2X + 5) and so spec(α) = {3 ± i, 1 ± 2i}.     −i i    1   1  1 1   √   0  , √2  0  2   0 0

The set  

  0  1  0  1  , √  , √   2 1  2 −i

 0    0   1    i

is an orthonormal basis for C4 composed of eigenvectors of α. (18.8) Proposition: Let V be a finitely-generated inner product space. Then the following conditions on a projection α ∈ End(V ) are equivalent: (1) α is normal; (2) α is selfadjoint; (3) ker(α) = im(α)⊥ . Proof: (1) ⇒ (2): From (1) we know that α(v) = α∗ (v) for all v ∈ V. In particular, α(v) = 0V if and only if α∗ (v) = 0V so that ker(α) = ker(α∗ ). If v ∈ V and w = v−α(v) then α(w) = α(v)−α2 (v) = α(v) − α(v) = 0V and so α∗ (w) = 0V . Therefore α∗ (v) = α∗ α(v) for all v ∈ V , whence α∗ = α∗ α. This implies that α = α∗∗ = (α∗ α)∗ = α∗ α∗∗ = α∗ α = α∗ , which proves (2). (2) ⇒ (3): If v, w ∈ V then, from (2), we see that α(v), w = v, α(w) . In particular, if v ∈ ker(α) then v, α(w) = 0 for all w ∈ V, which is to say that v ∈ im(α)⊥ . Conversely, if v ∈ im(α)⊥ then v, α(w) = 0 for all w ∈ V, which implies that α(v) is orthogonal to every element of V. Therefore α(v) = 0V and so v ∈ ker(α). This proves (3). (3) ⇒ (1): Let v, w ∈ V . Since α is a projection, we have v − α(v) ∈ ker(α). It is also clear that α(w) ∈ im(α). Therefore 0 = v − α(v), α(w) = v, α(w) − α(v), α(w) = v, α(w) − v, α∗ α(w) and since this is true for all v, w ∈ V, we have α = α∗ α. This implies that α = α∗ is selfadjoint and therefore surely normal, proving (1). We note that if V is a finitely-generated inner product space and if α ∈ End(V ) is normal, then, by Propositions 16.5, 16.7. and 18.5, we have V = ker(α) ⊕ im(α), and, in particular, {im(α), ker(α)} is an independent set of subspaces of V. Moreover, v ⊥ v for all v ∈ ker(α) and v ∈ im(α). While the direct-sum decomposition is valid for any projection, it is the nomality which ensures the orthogonality.


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(18.9) Proposition: Let V be a finitely-generated inner product space. Let W1 , . . . , Wn be subspaces of V and, for each 1 ≤ i ≤ n, let αi be the projection of V onto the subspace Wi coming from the decomposition V = Wi ⊕ Wi⊥ . Then the following conditions are equivalent: In , (1) V = Wi and Wh⊥ = j=h Wj for all 1 ≤ h ≤ n; i=1 (2) α1 + . . . + αn = σ 1 and αi αj = σ 0 for all i = j; (3) If Bi is an orthonormal basis of Wi for each i, then n B = i=1 Bi is an orthonormal basis of V. Proof: This has essentially already been established when we talked about the decomposition of a vector space into a direct sum of subspaces. (18.10) Proposition: Let F be either R or C and let V be a finitely-generated inner product space over F . If p(X) ∈ F [X] and if α is a normal endomorphism of V, then p(α) is a normal endomorphism of V. n n If p(X) = i=0 ai X i . Then p(α) = i=0 ai αi and p(α)∗ = Proof: n ∗ i ∗ ∗ i=0 ai (α ) . Since αα = α α, it follows from the definition of the ∗ ∗ product that p(α)p(α) = p(α) p(α). Therefore p(α) is a normal endomorphism of V. (18.11) Proposition: Let V be a finitely-generated inner product space and let α be a normal endomorphism of V. If the minimal polynomial of α is completely reducible, then it does not have multiple roots.

Proof: Let p(X) be the minimal polynomial of α, which we assume is completely reducible. Assume that there exists a scalar c and a polynomial q(X) such that p(X) = (X − c)2 q(X). Since p(α) = σ 0 , we have (α − cσ 1 )2 q(α) = σ 0 and so ker((α − cσ 1 )2 q(α)) = V. By Proposition 18.10, we know that β = α − cσ 1 is a normal endomorphism of V. Let v ∈ V and let w = q(α)(v). Then β 2 (w) = 0V and so β(w) ∈ im(β) ∩ ker(β) = {0V }. Thus we see that βq(α)(v) = 0V for all v ∈ V and hence α annihilates the polynomial (X − c)q(X), contradicting the minimality of p(X). (18.12) Proposition (Spectral Decomposition Theorem): Let V be an inner product space finitely generated over C and let α be a normal endomorphism of V . Then there exist scalars c1 , . . . , cn and projections α1 , . . . , αn of V satisfying: (1) α = c1 α1 + . . . + cn αn ;

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(2) σ 1 = α1 + . . . + αn ; (3) αh αj = σ 0 for all h = j. Moreover, these cj and αj are unique. The cj are precisely the distinct eigenvalues of α and each αj is the projection of V onto the eigenspace Wj associated with cj coming from the decomposition V = Wj ⊕ Wj⊥ . Proof: Let p(X) be nthe minimal polynomial of α, which we will write in the form p(X) = i=1 (X − ci ), where the ci are complex numbers which, by Proposition 18.11, are distinct. For each 1 ≤ j ≤ n, let pj (X) be the jth Langrange interpolation polynomial determined by the ci . Let f (X) be a polynomial of degree at most n − 1. Then the polyn nomial f (X) − i=1 f (ci )pi (X) is of degree at most n − 1 and has n distinct n and so nroots c1 , . . . , cn . Thus it must be the 0-polynomial f (c )p (X). In particular, we see that 1 = f (X) = i i i=1 n i=1 pi (X) n and X = i=1 ci pi (X). Set αj = pj (α). Then σ 1 = i=1 αi and n α = i=1 ci αi . Note that αj = σ 0 since αj = pj (α) and the degree of pj (X) is less than the degree of the minimal polynomial of α. Moreover, if h = j then there exists a polynomial u(X) ∈ C[X] satisfying u(α)σ 0 = σ 0 . Thus we see that for all 1 ≤ j ≤ n we αh αj = u(α)p(α) = n have αj = αj σ 1 = i=1 αj αi = α2j and so each αj is a projection. Thus we see that {im(αj ) | 1 ≤ j ≤ n} is an independent set of subspaces of V. Since the minimal polynomial and the characteristic polynomial of α have the same roots, we know that spec(α) = {c1 , . . . , cn }. To show that to im(αh )+ if Wh = im(αh ), we have to prove that a vector v belongs * n and only if α(v) = ch v. Indeed, if α(v) = ch v then ch j=1 αj (v) = n n ch v = α(v) = j=1 (cj αj )(v) and so j=1 [(ch − cj )αj ] (v) = 0V . Thus, for all j = h, we have αj (v) = 0V and so v = αh (v) ∈ im(αh ). Finally, we note that αh is the projection coming from the decomposition V = Wj ⊕ Wj⊥ since αh is a polynomial in α and hence normal and so the result follows from the remark after Proposition 18.8. Note that we could have deduced Proposition 18.12 directly from Proposition 18.7. What is important in the above proof is the explicit construction of the projection maps as polynomials in α. n n k α = i=1 ci αi is as in Proposition 18.12, then αk = ( i=1 ci αi ) = If n k integer k, and from this we see that if p(X) ∈ i=1 ci αi for any positive n C[X] then p(α) = i=1 p(ci )αi . (18.13) Proposition: Let V be an inner product space finitely generated over C. A normal endomorphism α of V is positive definite if and only if each of its eigenvalues is positive.


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Proof: If α is positive definite then, by Proposition 17.11, each of its eigenvalues is positive. Conversely, assume each of the eigenvalues of n α is positive. By Proposition 18.12, we write α = i=1 ci αi , where the ci are the eigenvalues of α and the αi are projections in End(V ) satisfying αi αj = σ 0 for i = j. If 0V = v ∈ V then α(v), v = n n n 2 i=1 j=1 ci αi (v), αj (v) = i=1 ci αi (v) > 0 and so α is positive definite. Example: Let V = R3 . For each a ∈ R, let αa ∈ End(V ) be the normal endomorphism of V represented with respect to the canonical   1 a a basis by the matrix  a 1 a  . Then spec(α) = {2a+1, 1−a} and so, a a 1 by Proposition 18.13, α is positive definite precisely when −1 < 2a < 2. As a consequence of Proposition 18.13 and the comments before it, we see that if α is a positive-definite endomorphism of a finitely-generated √ α inner product space V over C then there exists an endomorphism √ 2 √ of V satisfying ( α) = α. This endomorphism is defined by α= √ n ci αi , where the ci are the eigenvalues of α, and where the αi i=1 are defined as in Proposition 18.12. In particular, if β is an automorphism β ∗ β, which is also of V then, by Proposition 17.10, we can talk about positive definite by Proposition 18.13. (18.14) Proposition: Let V be an inner product space finitely generated over C and let α ∈ Aut(V ). Then there exists a unique positive-definite automorphism θ of V and a unique unitary automorphism ψ of V satisfying α = ψθ. Proof: By Proposition 17.10, we know that α∗ α of √ the automorphism −1 ∗ V is positive definite and so we can set θ = α α. Let ϕ = θα . Then ϕ∗ = (α−1 )∗ θ∗ = (α∗ )−1 θ so ϕ∗ ϕ = (α∗ )−1 θθα−1 = (α∗ )−1 α∗ αα−1 = σ 1 , proving that ϕ is unitary by Proposition 18.1, and hence belongs to Aut(V ). If we now define ψ = ϕ−1 , we see that α = ψθ. Moreover, we note that θ ∈ Aut(V ) since θ = ϕα. To prove uniqueness, assume that ψθ = ψ θ , where ψ and ψ are unitary automorphisms of V and where θ and θ are positive-definite automorphisms of V. Then ψ 2 = ψθ∗ θψ = ψ (θ )∗ θ ψ = (ψ )2 . Since ψ is positive definite, this implies that ψ = ψ and so, since ψ is an automorphism, we have θ = ψ −1 ψθ = ψ −1 ψθ = θ . The representation of an automorphism α of an inner product space finitely generated over C in the form given in Proposition 18.14 is sometimes

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called the polar decomposition of α. If we move over to matrices, we see that the polar decomposition of a nonsingular matrix A ∈ Mn×n (C) is of the form A = U M, where U is a unitary matrix and M is a Hermitian matrix satisfying the condition that vM v > 0 for all nonzero v ∈ Cn . Similarly, there exists a unitary matrix U and a Hermitian matrix M satisfying AH = U M and ao A = M (U )H , where (U )H is again unitary. In the case we are working over R, the matrix U is orthogonal, and M is symmetric and satisfies v T M v > 0 for all nonzero v ∈ Rn . Because polar decompositions are important in applications, several iterative algorithms exist to compute them. (18.15) Proposition (Singular Value Decomposition Theorem5 ): Let V and W be inner product spaces of finite dimensions k and n respectively, and let α ∈ Hom(V, W ). Then there exists an integer t ≤ min{k, n}, together with positive real numbers c1 ≥ c2 ≥ . . . ≥ ct and with orthonormal bases {v1 , . . . , vk } of V and {w1 , . . . wn } of W satisfying

ci wi if 1 ≤ i ≤ t α(vi ) = otherwise 0W and α∗ (wi ) =

ci vi 0V

if 1 ≤ i ≤ t . otherwise

Proof: If α is the 0-map, then the result is immediate, so assume that that is not the case. We note that β = α∗ α is a selfadjoint endomorphism of V and so, by Proposition 17.7, it is orthogonally diagonalizable. Hence V has an orthonormal basis {v1 , . . . , vk } composed of eigenvectors of β, where each vi is associated with an eigenvalue bi . By Proposition 17.10, we know that each bi belongs to R. Moreover, for each i we note that bi = bi vi , vi = bi vi , vi = β(vi ), vi = α(vi ), α(vi ) ≥ 0. Indeed, renumbering if necessary, we can assume that there exists an integer ≥ bt > 0 while bt+1 = . . . = bk = 0. t ≤ k such that b1 ≥ b2 ≥ . . . √ For each 1 ≤ i ≤ t, set ci = bi and let wi = c−1 i α(vi ) ∈ W. If

5 The first version of the Singular Value Decomposition Theorem was proven by the 19th-century Italian mathematician Eugenio Beltrami. It was subsequently extended by many others, including Camille Jordan and Sylvester.


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i = j then wi , wj = (ci cj )−1 α(vi ), α(vj ) = (ci cj )−1 β(vi ), vj = (ci cj )−1 bi vi , vj = 0 while, for each 1 ≤ i ≤ t, we have wi , wi = −2 −2 c−2 i α(vi ), α(vi ) = ci β(vi ), vi = ci bi vi , vi = vi , vi = 1. Thus we see that the set {w1 , . . . wt } is orthonormal. Moreover, for each 1 ≤ i ≤ t 2 we have α(vi ) = bi so α(vi ) = ci and α∗ (wi ) = α∗ c−1 i α(vi ) = −1 ∗ −1 −1 ci α α(vi ) = ci β(vi ) = ci bi vi = ci vi . For t + 1 ≤ i ≤ k we have α∗ α(vi ) = β(vi ) = 0V and so 0 = β(vi ), vi = α(vi ), α(vi ), which implies that α(vi ) = 0W . Thus vi ∈ ker(α) for each t + 1 ≤ i ≤ k. We are therefore left with the matter of defining wt+1 , . . . , wn in the case t < n. By Proposition 16.17, we know that ker(α∗ ) = im(α)⊥ and so, if we pick an orthonormal basis {wi+1 , . . . wn } for ker(α∗ ) we see that {w1 , . . . wn } is an orthonormal basis for W having the desired properties. The scalars c1 ≥ c2 ≥ . . . ≥ ct given in the Proposition 18.15 are called the singular values of the linear transformation α. The number c1 /ct , called the spectral condition number, is used as a measure of the numerical instability of the matrix representing α∗ α ∈ End(V ) with respect to the given basis. If we consider the special case of a linear transformation α : Ck → Cn represented with respect to the canonical bases by a matrix A ∈ Mn×k (C), the Singular Value Decomposition Theorem says that there exist unitary matrices P ∈ M ! n×n (C) and Q ∈ Mk×k (C) such that A can be written D O as P QH , where D ∈ Mt×t (R) is a diagonal matrix having the O O singular values of α on the diagonal. These singular values are precisely the square roots of the eigenvalues of AH A. The columns of Q form an orthonormal basis for Ck consisting of eigenvectors of AH A, and the columns of P form an orthonormal basis for Cn . If α : Rk → Rn then ! of course the matrices P and Q are orthogonal D O and A = P QT . O O   20 20 −20 20 1  1 17 1 −17  can be writExample: The matrix A = 10 18 6 18 −6     5 0 0 4 0 0 0 1 ten as a product P  0 3 0 0  Q, where P =  0 3 −4  5 0 4 3 0 0 2 0   1 1 −1 1  1 1 1 1 −1  are orthogonal and where the singular and Q =   1 1  2 1 −1 1 −1 −1 −1 values of A are 4, 3, 2.

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Singular value decompositions have many applications, and play important roles in the mathematics of optimization, of data compression, and of image processing. They are especially useful since accurate and relativelyefficient algorithms for computing these decompositions are readily available in many common linear-algebra software packages.

Exercises Exercise 989 Let A ∈ Mn×n (C) be similar to a unitary matrix. Is A−1 necessarily similar to AH ? Exercise 990 Let n > 1 be an integer and let V be the subspace of C[X] consisting of all polynomials of degree at most n. Let 0 = c ∈ C and let α be the endomorphism of V defined by α : p(X) → p(X + c). Is it possible to define an inner product on V relative to which α is normal? Exercise 991 Let a, b, c ∈ C. Find the set of all triples (x, y, z) of   a x y complex numbers satisfying the condition that the matrix  0 b z  0 0 c represents a normal endomorphism of C3 , endowed with the dot product, with respect to the canonical basis. Exercise 992 Let n be a positive integer. A matrix A ∈ Mn×n (C) is normal if and only if AH A = AAH . Show that every normal uppertriangular matrix is a diagonal matrix. Exercise 993 Let V = R2 , together with the dot product. Show that a matrix in M2×2 (R) is of the form ΦBB (α) for some normal endomorphism α of V which is not selfadjoint if and only if it is of the form ! a −b for real numbers a and b = 0. b a Exercise 994 Let V be an inner product space finitely generated over R and let S be the set of all isometries V . Is S an R-subalgebra of End(V )? Exercise 995 Let n be a positive integer and let V = Cn on which we have the dot product. If α ∈ End(V ), let G(α) = {α(v), v | v = 1}. For the special case n = 2, find G(α) and G(β), where α is represented


with respect to the canonical basis by the matrix

1 0 0 0

represented with respect to the canonical basis by the matrix

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! and β is ! 0 2 . 0 0

Exercise 996 Let V = R3 on which we have the dot product, and let W be the space of all polynomial functions in RR 4 of degree at most 1 2, on which we define the inner product f, g = 0 f (x)g(x)dx. Let   a b c α ∈ Hom(V, W ) be defined by α  b  : x → 1+ + +(b−c)x+cx2 . 2 6 c Is this linear transformation an isometry? Exercise 997 Let V be an inner product space and let α be an endomorphism of V satisfying the condition that α∗ α = σ 0 . Show that α = σ0 . Exercise 998 Let V = R3 with the dot product, and let α be the auto    a −c morphism of V defined by α :  b  →  −b  . Is α unitary? c −a   0 0 0 i  0 0 1 0   Exercise 999 Is the matrix   0 1 0 0  ∈ M4×4 (C) unitary? i 0 0 0 Exercise 1000 Find a real number a satisfying the condition that the   −9 + 8i −10 − 4i −16 − 18i 1 + 12i −10 − 4i  ∈ M3×3 (C) is unitary. matrix a  −2 − 24i 4 − 10i −2 − 24i −9 + 8i Exercise 1001 Find a real number a satisfying the condition that the   12 6 − 12i 12 + 6i 6 − 6i 1  a 5i 3 + i   6 + 12i  ∈ M4×4 (C) is unitary. matrix  12 − 6i −5i a 1 − 3i  24 6 + 6i 3−i 1 + 3i −22 Exercise 1002 Given a real number a, check if the matrix ! − sin2 (a) + i cos2 (a) (1 + i) sin(a) cos (a) ∈ M2×2 (C) (1 + i) sin(a) cos (a) − cos2 (a) + i sin2 (a) is unitary.

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Exercise 1003 Find all possible triples  1 −2 1 2 −1 exist, such that the matrix 3 a b

(a, b, c) of real numbers, if any  2 2  is orthogonal. c



 0.5 0.5 0.5 0.5  0.5 0.5 −0.5 −0.5   ∈ M4×4 (R) Exercise 1004 Is the matrix   0.5 −0.5 0.5 −0.5  0.5 −0.5 −0.5 0.5 orthogonal? ! c ∈ R2 , show that there exists an orthogonal d matrix A ∈ M2×2 (R) and a real number b satisfying the condition that ! b Av = . 0 Exercise 1005 If v =

Exercise 1006 Let a and b be real numbers, not both equal to 0.   ab a(a + b) b(a + b) 1  a(a + b) −b(a + b) ∈ ab Show that the matrix 2 a + ab + b2 b(a + b) ab −a(a + b) M3×3 (R) is orthogonal. 

 2a −2a a Exercise 1007 Find all a ∈ R such that the matrix  −2a −a 2a  ∈ a 2a 2a M3×3 (R) is orthogonal. 

4 −1 4 Exercise 1008 Let A =  −1 1 −1

 1 −1  ∈ M3×3 (R). Find an or4

thogonal matrix P such that P T AP is a diagonal matrix. 

1  0 Exercise 1009 A =   0 0

0 0 1 0

0 1 0 0

 0 0   ∈ M4×4 (R). Find an orthogonal 0  1

matrix P such that P T AP is a diagonal matrix. Exercise 1010 Let n be a positive integer and let A and B be orthogonal matrices in Mn×n (R) satisfying |A| + |B| = 0. Show that |A + B| = 0.


 1 −1 √ 1 √ Exercise 1011 Let A = 2 2 2 2 2 −1 1

387

√  2 2 0  ∈ M3×3 (R). Find an √ 2 2

infinite number of pairs (P, Q) of orthogonal matrices such that is a diagonal matrix.  a − 45 4  a Exercise 1012 Find an a ∈ R such that the matrix 5 0 0 M3×3 (R) is orthogonal.

P AQ  0 0 ∈ 1

Exercise 1013 Let A, B ∈ Mk×n (R) be matrices such that the columns of each form orthonormal bases for the same subspace W of Rk . Show that AAT = BB T . Exercise 1014 Let ! A, B ∈ Mn×n (R) be orthogonal matrices. Is the A O matrix ∈ M2n×2n (R) necessarily orthogonal? O B Exercise 1015 Let n be a positive integer and let A ∈ Mn×n (R) be a skew-symmetric matrix. Show that (A − I)−1 (A + I) is an orthogonal matrix which does not have 1 as an eigenvalue.   0       0  4 Exercise 1016 Find two distinct functions f1 , f2 : R   0  → R      0 satisfying the condition that     2 a 2 2 2 2(bc − da) 2(bd − ca)  b  a + b − c − d     2(cd − ba) 2(bcda) a2 + b2 − c2 − d2 fi   c  2 2 2 2 2(bd − ca) 2(cd − ba) a +b −c −d d is always an orthogonal matrix. Exercise 1017 Let O = A ∈ M3×3 (C) be a matrix satisfying adj(A) = AH . Show that A is a unitary matrix having determinant 1. Exercise 1018 Let n be a positive integer and let α be the endomorphism of Cn defined by α : v → iv. Is α normal? Exercise 1019 Let V be an inner product space and let α, β ∈ End(V ) be normal. Is βα necessarily normal? Exercise 1020 Let V be an inner product space finitely-generated over C and let α ∈ End(V ) satisfy the condition that every eigenvector of β = α + α∗ is also an eigenvector of γ = α − α∗ . Prove that α is normal.

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α be the endomorphism of C2 represented with ! 2 i respect to the canonical basis by the matrix A = . Is α normal? i 2

Exercise 1021 Let

Exercise 1022 Let V be an inner product space over C and let α ∈ End(V ) be normal. If c ∈ C, is the endomorphism α − cσ 1 necessarily normal? Exercise 1023 Let V be an inner product space finitely generated over C and let σ 0 = α ∈ End(V ) be normal. Show that α is not nilpotent. 3 Exercise 1024 Let a, b ∈ R let α ∈ End(R  ) be represented with respect a −2 b a −2  . For which values of a and to the canonical basis by  b −2 3 a b is this endomorphism normal?

α ∈ End(R3 ) be represented with respect to the   14 2 14 canonical basis by the matrix 13  2 −1 −16  . Show that α is 14 −16 5 Exercise 1025 Let

selfadjoint and find an orthonormal basis of R3 composed of eigenvectors of α. α be the endomorphism of C3 represented with   6 −2 3 6 −2  . Show respect to the canonical basis by the matrix  3 −2 3 6 Exercise 1026 Let

that α is normal and find an orthonormal basis of C3 eigenvectors of α.

composed of

Exercise 1027 Let V be an inner product space and let σ 0 = α ∈ End(V ) be a normal projection. Show that α(v) ≤ v for all v ∈ V, with equality whenever v ∈ im(α). Give an example where this does not hold for α which is not normal.     a1 a1  a2    a2    Exercise 1028 Let α ∈ End(R4 ) be defined by α :   a3  →  a3 + a4  . a4 a4 − a3 Show that α is normal but not selfadjoint.

19 Moore-Penrose pseudoinverses

Let V and W be inner product spaces, and let α : V → W be a linear transformation. We know that there exists a linear transformation β : W → V satisfying the condition that βα is the identity function on V and αβ is the identity function on W if and only if α is an isomorphism; in this case, β = α−1 . If both spaces are finitely generated, we also know that such an isomorphism can exist only when dim(V ) = dim(W ). If α is not an isomorphism, it is possible to weaken the notion of the the inverse of a function. Given a linear transformation α : V → W, we say that a linear transformation β : W → V is a Moore-Penrose1 pseudoinverse of α if and only if the following conditions are satisfied: (1) αβα = α and βαβ = β; (2) The endomorphisms βα ∈ End(V ) and αβ ∈ End(W ) are selfadjoint.

1

Eliakim Hastings Moore developed this construction in 1922, but it did not receive much attention at the time; it was rediscovered independently in 1955 by Sir Roger Penrose, a contemporary British applied mathematician, best known for his collaboration with the physicist Stephen Hawking.

389

390

19. Moore-Penrose pseudoinverses

Example: The two parts of condition (2) in the definition of the MoorePenrose pseudoinverse are independent. To see this, consider the linear ! 1 2 3 3 2 v. For transformation α : R → R defined by α : v → 0 1 0 any c, d ∈ R, let β : R2 → R3 be the linear transformation defined   1 − 3c −2 − 3d  . Then one can check that αβα = α 0 1 by β : w →  c d and βαβ = β and that αβ = σ 1 in End(R2 ). On the other hand,   1 − 3c −6c − 3d 3 − 9c  v, and it is easy enough to choose 0 1 0 βα : v →  c 2c + d 3c c and d so that this matrix is not symmetric and hence βα is not selfadjoint. We will denote the Moore-Penrose pseudoinverse of α by α+ . Of course, in order to justify this notation we have to show that β exists and is unique, which we will do for the case that V and W are finitely generated. We will begin with uniqueness. (19.1) Proposition: Let V and W be inner product spaces and let α : V → W be a linear transformation. If α has a Moore-Penrose pseudoinverse, it must be unique. Proof: Suppose that β, γ ∈ Hom(W, V ) are Moore-Penrose pseudoinverses of α. Then β = βαβ = (βα)∗ β = α∗ β ∗ β = (αγα)∗ β ∗ β = (γα)∗ α∗ β ∗ β = γαα∗ β ∗ β = γα(βα)∗ β = γαβαβ = γαβ = γαγαβ = γ(αγ)∗ αβ = γγ ∗ α∗ αβ = γγ ∗ α∗ (αβ)∗ = γγ ∗ (αβα)∗ = γγ ∗ α∗ = γ(αγ)∗ = γαγ = γ and so we have proven uniqueness. In particular, if α : V → W is an isomorphism, then, by Proposition 19.1, we have α+ = α−1 . If α is the 0-function then so is α+ . (19.2) Proposition: Let V and W be finitely-generated inner product spaces and let α : V → W be a linear transformation. (1) If α is a monomorphism, then α+ exists and equals (α∗ α)−1 α∗ . Moreover, α+ α is the identity function on V ; (2) If α is an epimorphism, then α+ exists and equals ∗ α (αα∗ )−1 . Moreover, αα+ is the identity function on W. Proof: (1) From Proposition 16.19, we see that if α is a monomorphism then α∗ α ∈ Aut(V ) and so (α∗ α)−1 exists. Set β = (α∗ α)−1 α∗ . Then


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βα is the identity function on V and so βα is a selfadjoint endomorphism of = β. Finally, (αβ)∗ = ( V∗ which ) satisfies ) = α and ∗ βαβ ( ∗ αβα −1 ∗ ∗ −1 ∗ ∗ ∗ −1 ∗ α(α α) α = α (α α) α = α [(α α) ] α = α(α∗ α)−1 α∗ = αβ and so αβ is also selfadjoint. Thus β = α+ . (2) From Proposition 16.19, we see that if α is an epimorphism then αα∗ ∈ Aut(W ) and so (αα∗ )−1 exists. As in (1), we see that α∗ (αα∗ )−1 = α+ . Example: Let α : R2 → R3 be the linear transformation represented   1 2 with respect to the canonical bases by the matrix  −1 3  . This is a 2 4 monomorphism and so, by Proposition 19.2, α+ exists and is represented ! 1 3 −10 6 . with respect to the canonical bases by the matrix 5 2 25 1 (19.3) Proposition: Let V and W be finitely-generated inner product spaces. Then every α ∈ Hom(V, W ) has a Moore-Penrose pseudoinverse α+ ∈ Hom(W, V ). Proof: Let Y = im(α), and write α = µβ, where β : V → Y is an epimorphism given by β : v → α(v), and µ : Y → W is the inclusion monomorphism. By Proposition 19.2, we know that β + ∈ Hom(Y, V ) and µ+ ∈ Hom(W, Y ) exist and satisfy the conditions that ββ + and µ+ µ are equal to the identity function on Y. Therefore we see that (µβ)(β + µ+ )(µβ) = µβ and (β + µ+ )(µβ)(β + µ+ ) = β + µ+ and we see that (β + µ+ )(µβ) = β + β and (µβ)(β + µ+ ) = µµ+ are selfadjoint. Thus α+ exists and equals β + µ+ . As an immediate consequence of this, we note that if α is an endomorphism of a finitely-generated inner produce space V then, by Proposition 6.11, we see that rk(αα+ ) ≤ rk(α) and rk(α) = rk(αα+ α) ≤ rk(αα+ ) and so rk(αα+ ) = rk(α). Similarly, rk(α+ α) = rk(α). If F is either R or C, and if we are given a linear transformation α : F k → F n which is represented with respect to the canonical bases by the matrix A = [aij ], then we will denote the matrix representing α+ with respect to these bases by A+ . Thus the matrix A+ has the following properties: (1) AA+ A = A and A+ AA+ = A+ ; (2) The matrices AA+ and A+ A are symmetric (in the case F = R) or Hermitian (in the case F = C).

392




 1 −1 2 1 −2  ∈ M3×3 (R). This matrix is Example: Let A =  2 3 0 0 clearly singularand hence A−1 does not exist. However, we can check 5 5 10 1  −5 4 −1  . that A+ = 45 10 −8 2 For nonsingular square matrices of the same size A and B, we know that (AB)−1 = B −1 A−1 . A similar equality does not hold for the MoorePenrose pseudoinverse, as the following example shows. ! ! 2 6 1 2 Example: If A = and B = in M2×2 (R), then 1 3 2 4 ! ! ! 1 1 2 1 1 2 14 28 + + and B = AB = . Then A = 7 14 50 6 3 25 2 4 ! ! 7 1 2 1 2 1 , while (AB)+ = . so B + A+ = 1250 4 2 175 4 2 ! 1 0 Example: If A(t) = for all real numbers t then we see 0 t ! ! 1 0 1 0 that A(t)+ = when t = 0, but is equal to for 0 0 0 t−1 t = 0. Thus we see that not only is lim A(t) not equal to A(0), but t→0

indeed that the value of A(t) moves farther and farther away from A(0) as t approaches 0. Thus we see that the Moore-Penrose pseudoinverse is not computationally stable. This means that one has to be very careful in actual applications. Because of the importance and utility of Moore-Penrose pseudoinverses, there exists a considerable literature on techniques for computing A+ or A+ A, given a matrix A. One of the methods used in practice for computing the Moore-Penrose pseudoinverse over R is a recursive one, known as Greville’s method2 , which is based on the following result: if

2 In the 1970’s, American mathematician Thomas N. E. Greville and American/Israeli mathematician Adi Ben-Israel popularized and reinvigorated the use of the Moore-Penrose pseudoinverse as a computational tool.


393

( ) A ∈ Mk×n (R), and if we write!A = B v , where B ∈ Mk×(n−1) (R), B + (I − v ∧ w) then A+ = , where w   ((I − BB + )v)−2 (I − BB + )v if (I − BB + )v = 0 −1 . w=  1 + B + v2 (B + )T B + v otherwise

Another technique is to break A up into blocks, if possible. Indeed, if ! A11 A12 , where A11 is a nonsingular square matrix the rank A= A21 A22 of which equals the rank of A, then, by Zlobec’s formula, we have A+ = ! !−1 )∗ ∗ A11 ∗ ) ( ( A11 A11 A12 A11 A12 A∗ B , where B = . A21 A21 One can also use convergence methods to compute the Moore-Penrose pseudoinverse of a matrix. If A ∈ Mk×n (C) then, by Proposition 17.4, we know that the eigenvalues of A∗ A are real. Let c be the largest such eigenvalue and pick a real number b satisfying 0 < bc < 2. For each integer p ≥ 2, define the sequence Y0 , Y1 , . . . of matrices in Mn×k (C) as follows: (1) Y0 = bA∗ ; (2) If k ≥ 0 and Yk has already been defined, set Tk = I − Yk A and p−1 set Yk+1 = Yk + i=1 Tki Yk . Then the sequence Y0 , Y1 , . . . converges to A+ . Another method is the following: if A ∈ Mn×n (R) is an arbitrary symmetric matrix we can define matrices A0 , A1 , . . . by setting A0 = A ) ( and Ak+1 = I + (I − Ak )(I + Ak )−1 Ak for all k ≥ 0. Also, we can define real numbers c0 , c1 , . . . by setting c0 = 1 and ci+1 = 2ci + 1 for each i ≥ 0. Then the Kovarik algorithm states that if none of the is an eigenvalue of A, the sequence A0 , A1 , . . . converges numbers −c−1 i to A+ A. Let F be either R or C, let k and n be positive integers, and let A ∈ Mk×n (F ). We now look at what the matrix A+ says about a solution (if any) to a system of linear equations of the form AX = w, where w ∈ F k . First of all, we note that in general (19.4) Proposition: Let F be either R or C, let k and n be positive integers, let A ∈ Mk×n (F ), and let w ∈ F k . The system of linear equations AX = w has a solution if and only if (AA+ )w = w.

394


Proof: If there is a vector v ∈ F n satisfying Av = w then (AA+ )w = (AA+ )(Av) = (AA+ A)v = Av = w. Conversely, if (AA+ )w = w then A(A+ w) = w and so Av = w, where v = A+ w.

n +  Wealso note that, in the situation above, if y ∈ F then A(I −A A)y = 0  ..   .  and so we also see that A+ w + (I − A+ A)y is also a solution to

0 the system AX = w, assuming that the system has any solutions at all. Conversely, any solution to this system is of the form A+ w + u, where   0  ..  Au =  .  , and so (I − A+ A)u = u. 0 (19.5) Proposition: Let F be either R or C, let k and n be positive integers, and let A ∈ Mk×n (F ). Let w ∈ F k . If the system AX = w has a solution then in the set of all solutions to this system of linear equations there is precisely one having a minimal norm, and it is A+ w. Proof: If u is a solution to this system, then we have already seen that it is of the form A+ w + (I − A+ A)y. But we note that E + F A w, (I − A+ A)y

E + F A AA+ w, (I − A+ A)y F E = A+ w, (A+ A)(I − A+ A)y F E = A+ w, (A+ A − A+ AA+ A)y   8 0 9   = A+ w,  ...  = 0 0 =

so 2

u

E F u, u = A+ w + (I − A+ A)y, A+ w + (I − A+ A)y F E F E = A+ w, A+ w + (I − A+ A)y, (I − A+ A)y >2 > >2 > = >A+ w> + >(I − A+ A)y > ,

=

which implies that u ≥ A+ w .


395

! ! 2 −1 1 1 Example: Let A = and w = . Then A+ = 1 1 1 2   4 2 1  −5 8  and so the solution to the system AX = w having minimal 14 1 4   8 √ 1  11  . Its norm is 1 266. norm is A+ w = 14 14 9 But what happens if the system AX = w doesn’t have a solution? Suppose that F is either R or C and that A ∈ Mk×n (F ), and w ∈ F k , where k and n be positive integers. Then the system (A+ A)X = A+ w always has a solution, namely A+ w, and by Proposition 19.5 this is in fact the solution of minimal norm of this equation, which is the best approximation to a solution of AX = w. In order to emphasize the use of Proposition 19.5, we briefly consider the least squares method, which is an important tool in many areas of applied mathematics and statistics. This method was developed at the beginning of the nineteenth century by Gauss and Legendre and, independently, by the American mathematical pioneer Robert Adrain3 . Suppose that we have before us the results of several observations, which, depending on values t1 , . . . , tn of a real parameter, give us real values c1 , . . . , cn . Our theory tells us that the set of points {(ti , ci ) | 1 ≤ i ≤ n} in the euclidean plane should lie on a straight line. However, because of measuring and/or computational errors, this doesn’t quite work out. So we want to find the equation of the line in the plane which best fits our observed data. In other words, we want to find a solution of minimal norm to the system of linear equations {X1 + ti X2 = ci | 1 ≤ i ≤ n}, which can be     c1 1 t1 !  c   1 t2   2    X1 =  .  . As we have seen, the solution written as  . .  . .  ..   . .  X2 1

tn

cn

3 Irish-born Robert Adrain emigrated to the United States in 1798. He published his own mathematics journal but his work received no international attention at the time.

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   of minimal norm, if it exists, is  

1 1 .. .

t1 t2 .. .

+     

1 tn

   

c1 c2 .. .

    . Otherwise, this is 

cn

the best approximation to the solution the system. Example: To find the equation of the line in the euclidean plane which best fits the set of points {(1, 3), (2, 7), (3, 8), (4, 11)}, we calculate 

1  1   1 1

+  3 1  7 2    3   8 11 4

  = 

1 20

20 10 0 −6 −2 2

−10 6

!



 3  7  1    8 = 2 11

2 5

!

so the line we want is given by {(t, 1 + 52 t) | t ∈ R}. We can use the same method to find the best fit of any polynomial of a higher degree to a set of points. For example, if we wish to find a parabola which best fits the set of points {(ti , ci ) | 1 ≤ i ≤ n} in the euclidean plane, we have to find a best approximation to a solution of the system of linear equations {X1 + ti X2 + t2i = ci | 1 ≤ i ≤ n}, which we know is +    c1 1 t1 t21  1 t2 t22   c2       .. .. ..   ..  .    . . . .  1

tn

t2n

cn

Example: To find the equation of the parabola in the euclidean plane which best fits the set of points {(1, 3), (2, 7), (3, 8), (4, 11)}, we calculate 

1  1   1 1

+  3 1 1  7 2 4    3 9   8 11 4 16

   

  45 −15 −25 15  1 23 27 −19   =   −31  20 5 −5 −5 5   −1 1 15  . = 4 −1 



and so the parabola we want is given by {(t, − 14 +

15 4 t

 3 7   8  11

− 14 t2 ) | t ∈ R}.

Needless to say, we can also consider a much more general context. Suppose that W is a finitely-generated subspace of RA . Given a set of observations {(ti , ci ) | 1 ≤ i ≤ n} ⊆ A × R, we want to find the function g ∈ W which best approximates these observations.


397

To do this, we pick a basis {f1 , . . . fk } for W . Then we want to find a best approximation to a solution of the system of linear equations {X1 f1 (ti ) + . . . Xk fk (ti ) = ci | 1 ≤ i ≤ n},     f1 (t1 ) . . . fk (t1 ) X1    ..   .. .. which can be written as   .  =  . .   we have seen, this is 

f1 (tn ) . . . f1 (t1 ) .. .

...

f1 (tn ) . . .

fk (tn ) +  fk (t1 )   ..   .

fk (tn )

Xk 

 c1 ..  . As .  cn

c1 ..  . .  cn

Least-squares approximations are often used to find best-fit solutions to very large systems of linear equations of the form AX = w which, in theory, have an exact solution but in practice that solution cannot be found because of errors in measurement of the data and computational errors. Indeed, Gauss developed this method for finding solutions to the very large systems of linear equations which resulted from laying down a triangulation grid for a geodetic survey of the state of Hanover he conducted in 1818. In 1978, the American National Geodetic Survey used it to solve a system of over 2.5 million linear equations in 400,000 unknowns which resulted from the updating of the triangulation grid for the continental United States.

Exercises 

Exercise 1029 Exercise 1030 Exercise 1031 positive integer. Exercise 1032

 1 1 Let A =  −1 1  ∈ M3×2 (R). Calculate A+ . 2 3 ( ) Let A = 5 0 0 ∈ M1×2 (Q). Calculate A+ . ) ( ∈ M1×n (C), where n is a Let A = a1 . . . an Show that A+ = (AAH )−1 AH .   2 2 0 Let A =  1 2 1  ∈ M3×3 (R). Calculate A+ . 1 2 1

Exercise 1033 Let V and W be finitely-generated inner product spaces, and let α ∈ Hom(V, W ). For any nonzero scalar c, show that (cα)+ = 1 + cα .

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Exercise 1034 Let n be a positive integer and let A ∈ Mn×n (R) be a diagonal matrix. Calculate A+ . Exercise 1035 Let V and W be finitely-generated inner product spaces, and let α ∈ Hom(V, W ). Show that (α∗ )+ = (α+ )∗ . Exercise 1036 Let V = R2 , which is endowed with the dot !product and a let α : V → R be the linear functional defined by α : → a. Let b ! a β : R →V be the linear transformation defined by β : a → . Show a that (αβ)+ = β + α+ . Exercise 1037 Let n be a positive integer and let A = [aij ] ∈ Mn×n (R) be the matrix all entries of which are equal to 1. Show that A+ = n−2 A. ! C O , Exercise 1038 Let A ∈ Mk×n (R) be a matrix of the form O O where C is a t × t nonsingular diagonal matrix. Show that A+ = ! D O , where D = C −1 . O O Exercise 1039 Let V = Rn on which we have the dot product defined, and let α ∈ End(V ) satisfy the condition that ker(α) = im(α)⊥ . Show that the restriction β of α to im(α) is an automorphism of im(α) and that the restriction of α+ to im(α) equals β −1 . Exercise 1040 Let n be a positive integer and let A, B ∈ Mn×n (R) be matrices satisfying the conditions ABA = A, BAB = B, and A2 = A. Is it necessarily true that B 2 = B? Exercise 1041 Let h, k, m, and n be positive integers, let A ∈ Mh×k (R), let B ∈ Mm×n (R), and let C ∈ Mh×n (R). Show that there exists a matrix X ∈ Mk×m (R) satisfying AXB = C if and only if AA+ CB + B = C. Exercise 1042 Let k and n be positive integers and let B ∈ Mk×k (R) and C ∈ Mn×n (R) be orthogonal matrices. For A ∈ Mk×n (R), show that (BAC)+ = C T A+ B T . Exercise 1043 Let k and n be positive integers and let A ∈ Mk×k (R) and B ∈ Mk×n (R). Let C ∈ Mn×n (R) be nonsingular. Prove that A O

AB C

!+ =

A+ O

−A+ ABC −1 C −1

! .

20 Bilinear transformations and forms

Let V, W, and Y be vector spaces over a field F. We say that a function f : V × W → Y is a bilinear transformation if and only if the function v → f (v, w0 ) belongs to Hom(V, Y ) for any given vector w0 ∈ W and the function w → f (v0 , w) belongs to Hom(W, Y ) for any given vector v0 ∈ V. The set of all bilinear transformations from V × W to Y will be denoted by Bil(V × W, Y ). If f, g ∈ Bil(V × W, Y ) and if c ∈ F then f + g and cf also belong to Bil(V × W, Y ), and so Bil(V ×W, Y ) is a subspace of the vector space Y V ×W over F. Also, any bilinear transformation f : V × W → Y defines a bilinear transformation f op : W × V → Y, called the opposite transformation of f, by setting f op : (w, v) → f (v, w). It is clear that the function ( )op : Bil(V × W, Y ) → Bil(W × V, Y ) is an isomorphism of vector spaces. We say that a bilinear transformation f ∈ Bil(V × V, Y ) is symmetric if and only if f = f op . In particular, if we consider a single vector space V over a field F, then we note that f ∈ Bil(V × V, V ) if and only if the operation • on V defined by v • w = f (v, w) turns V into an F -algebra. This algebra is commutative if and only if f is symmetric. Example: Let F be a field and let k, n, and t be positive integers. Set V = Mk×n (F ), W = Mt×n (F ), and Y = Mk×t (F ). Then there 399

400

20. Bilinear transformations and forms

exists a bilinear transformation V × W → Y defined by (A, B) → AB T . In particular, we have a bilinear transformation F n × F n → Mn×n (F ) given by (v, w) → v ∧ w. More generally, if V, W, and Y are as mentioned, every matrix C ∈ Mn×n (F ) defines a bilinear transformation V × W → Y by setting (A, B) → ACB T . Example: For vector spaces V and W over a field F, the function Hom(V, W )×V → W given by (α, v) → α(v) is a bilinear transformation. Let V, W, and Y be vector spaces over a field F. The image of a bilinear transformation f ∈ Bil(V × W, Y ) is not necessarily a subspace of Y, as the following example shows. Example: Consider the bilinear transformation f : R2 ×R2 → M2×2 (R) ! 0 1 defined by f : (v, w) → v ∧ w. The image of f contains and 0 0 ! ! 0 0 0 1 , but is not a subspace since ∈ / im(f ). 1 0 1 0 As with linear transformations, bilinear transformations are totally determined by their behavior on bases. That is to say, let V and W be vector spaces over a field F, and let B = {vi | i ∈ Ω} and D = {wj | j ∈ Λ} be bases of V and W respectively. Let Y be a vector space over F and let f0 : B × D → Y be a function. Then there exists a unique bilinear transformation f ∈ Bil(V ×W, Y ) satisfying all i and j, namely the function defined by f (v i , wj ) = f0 (vi , wj ) for a v , b w f: i∈Ω i i j∈Λ j j → i∈Ω j∈Λ ai bj f0 (vi , wj ). In the case that V = W = Y, we have already noted this fact in Proposition 5.5. (20.1) Proposition: If V, W, and Y are vector spaces over a field F, then Bil(V × W, Y ) is isomorphic to Hom(V, Hom(W, Y )). Proof: Define a function θ : Bil(V ×W, Y ) → Hom(V, Hom(W, Y )) as follows: given a bilinear transformation f ∈ Bil(V × W, Y ) and a vector v ∈ V, then θ(f )(v) : w → f (v, w). It is straightforward to check that indeed θ(f )(v) ∈ Hom(W, Y ) for all f ∈ Bil(V × W, Y ) and all v ∈ V. Moreover, θ(f )(v1 + v2 ) = θ(f )(v1 ) + θ(f )(v2 ) and θ(f )(cv) = cθ(f )(v) for all v, v1 , v2 ∈ V and all c ∈ F, so θ(f ) ∈ Hom(V, Hom(W, Y )) for all f ∈ Bil(V × W, Y ). Finally, θ(f + g) = θ(f ) + θ(g) and θ(cf ) = cθ(f ) for all f, g ∈ Bil(V × W, Y ) and all c ∈ F, and so we have shown that θ is a linear transformation. It is also possible to define a function ϕ : Hom(V, Hom(W, Y )) → Bil(V × W, Y )


401

by setting ϕ(α) : (v, w) → α(v)(w) for all v ∈ V and w ∈ W, and again it is easy to show that this is a linear transformation. If α ∈ Hom(V, Hom(W, Y )) and v ∈ V, then θϕ(α)(v) : w → ϕ(α)(v)(w) = α(v)(w) and so θϕ(α)(v) = α(v) for all v ∈ V. Thus θϕ(α) = α for all α ∈ Hom(V, Hom(W, Y )), and so θϕ is the identity function on Hom(V, Hom(W, Y )). Conversely, if f ∈ Bil(V × W, Y ) then ϕθ(f ) : (v, w) → θ(f )(v)(w) = f (v, w) for all v ∈ V and w ∈ W and so ϕθ(f ) = f for all f ∈ Bil(V × W, Y ), proving that ϕθ is the identity function on Bil(V × W, Y ). Thus we have established that θ is an isomorphism, with θ−1 = ϕ. Let V and W be vector spaces over a field F. A bilinear transformation f : V × W → F is called a bilinear form. We will denote the set of all such bilinear forms by Bil(V ×W ), instead of Bil(V ×W, F ). By what we have seen above, Bil(V ×W ) is a subspace of F V ×W which is isomorphic to Hom(V, D(W )). If V and W are vector spaces over a field F, then a bilinear form f ∈ Bil(V, W ) is nondegenerate if and only if for each 0V = v ∈ V there exists a w ∈ W satisfying f (v.w) = 0 and for each 0W = w ∈ W there exists a v ∈ V satisfying f (v.w) = 0. Example: If V is an inner product space over R, then the function (v, w) → v, w belongs to Bil(V × V ). This is not true, of course, if our field of scalars is C. Example: If F is a field and V = F n for some positive integer n, then the function (v, w) → v w belongs to Bil(F n × F n ). This function is particularly useful in the case F = GF (2). Indeed, if v ∈ GF (2)n , then

0 if an even number of entries in v are equal to 1 vv = . 1 if an odd number of entries in v are equal to 1 This value is known as the parity of v. More generally, let A be a finite set and let V be the collection of all subsets of A. Define a bilinear form f : V × V → GF (2) by setting

0 if A ∩ B has an even number of elements f (A, B) = . 1 if A ∩ B has an odd number of elements Then f ∈ Bil(V, V ). Example: If V is a vector space over a field F , we have a nondegenerate bilinear form in Bil(D(V ) × V ) given by (δ, v) → δ(v). Similarly, if δ 1 , δ 2 ∈ D(V ), we have a bilinear form in Bil(V × V ) given by (v, w) → δ 1 (v)δ 2 (w), which is nondegenerate if δ 1 and δ 2 are not the 0-functional.

402


Example: If F is a field and if k and n are positive integers, then each matrix A ∈ Mk×n (F ) defines a bilinear form in Bil(F k × F n ) by (v, w) → v Aw. If V and W are vector spaces of finite dimension k and n respectively over F, then any bilinear form on V × W can be represented as in the previous example. Indeed if we fix bases B = {v1 , . . . , vk } for V and D = {w1 , . . . , wn } for W, then for any f ∈ Bil(V × W ) we define the k ) = [f (vi , wj )] ∈ Mk×n (F ) and check that if v = i=1 ai vi matrix TBD (f n and w = j=1 bj wj , then f (v, w) = v TBD (f )w. Indeed, for fixed B and D, the function f → TBD (f ) is an isomorphism from Bil(V × W ) to Mk×n (F ). Example: Let F be a field and let V = F 2 . Consider the bases

! ! ! !1 0 1 1 B= , and D = , of V. If f ∈ Bil(V, V ) 0 −1 1  1 ! ! a c  , → (a + b)(c + d), then it is easy to verify is given by f :  b d that TBB (f ) =

1 1 1 1

! and TDD (f ) =

0 0

0 4

! .

(20.2) Proposition: Let V and W be vector spaces finitely generated over a field F and having bases B = {v1 , . . . , vk } and D = {w1 , . . . , wn } respectively. Let C = {x1 , . . . , xk } and E = {y1 , . . . , yn } also be bases for V and W respectively, and let P = [pir ] ∈ Mk×k (F ) and Q = [qjs ] ∈ Mn×n (F ) be nonsingular         x1 v1 y1 w1         matrices satisfying  ...  = P  ...  and  ...  = Q  ...  . xk vk yn wn Then for f ∈ Bil(V × W ) we see that TCD (f ) = P TBD (f )QT . Proof: As a direct consequence of the definitions, we see that # " k n n k pir vr , qjs ws = pir f (vr , ws )qjs , f (xi , yj ) = r=1

s=1

r=1 s=1

and this is precisely the (i, j) entry of P TBD (f )QT .

In particular, we see that if f ∈ Bil(V × V ), where V is a vector space of finite dimension n over a field F, and if B and D are bases of V, then there exists a nonsingular matrix P ∈ Mn×n (F ) satisfying


403

TDD (f ) = P TBB (f )P T . In general, matrices A and C in Mn×n (F ) are congruent if and only if there exists a nonsingular matrix P ∈ Mn×n (F ) satisfying C = P AP T . Congruence is easily checked to be an equivalence relation on Mn×n (F ), which joins the relations of equivalence and similarity, that we have already defined. Congruent matrices clearly have the same rank, so that the rank of a matrix of the form TBB (f ) depends only on f and not on the choice of basis B. Therefore we call this the rank of the bilinear form f. Thus, for example, the bilinear forms in Bil(V × V ) of rank 1 are precisely those of the form (v, w) → α(v)β(w), where α, β ∈ D(V ). A matrix congruent to a symmetric matrix is again symmetric. Indeed, if A ∈ Mn×n (F ) is symmetric, then for any nonsingular matrix P we have (P AP T )T = P T T AT P T = P AP T .   1 −6 −6 Example: The matrix A =  −6 40 39  ∈ M3×3 (R) is congru−6 39 39  1 0 0 1  3 0  . 2 ent to I, since P AP T = I, where P =    √ √ √ 3 − 23 2 3 3 As was the case with inner products, we can define orthogonality with respect to an arbitrary bilinear form. This concept has important applications when we are working over fields other than R or C, and especially in areas such as algebraic coding theory, where all of the work is done over finite fields. Let V be a vector space over a field F and let f ∈ Bil(V ×V ). Vectors v, w ∈ V are f -orthogonal if and only if f (v, w) = 0. In this case, we will write v ⊥f w. (One has to be careful here, it may be true that v ⊥f w but false that w ⊥f v; this will not happen, of course, if f is symmetric.) If A is a nonempty subset of V , then we can talk about the right f -orthogonal complement of A to be the set A⊥f = {w ∈ V | v ⊥f w for all v ∈ A}. Complements of this form may behave very differently than complements defined by inner products, as the following example shows. Example: Let F = GF (2) and let V = F 4 . Define f      0 1       0  , 1 , by setting f (v, w) = v w. Then W =     0 1      0 1

∈ Bil(V × V )    1 0    1  0  ,  1   0    0 1

is a subspace of V which satisfies W ⊥f = W. We note that V ⊥f is trivial if and only if for any 0V = w ∈ V there exists a vector v ∈ V satisfying f (v, w) = 0. This condition is not a

404


consequence of our definitions, and we must explicitly state it when we need it. It holds, of course, if f is nondegenerate.     1 1         1   1    Example: Let V = R   ,  ⊆ R4 . If f ∈ Bil(V × V ) 1 −1       1 −1     a1 b1  a2   b2      is defined by f :   a3  ,  b3  → a1 b1 + a2 b2 + a3 b3 − a4 b4 , then a4 b4       1 0 0       0     −1   ∈ V ⊥f and, indeed, V ⊥f = R  , 0  .  0   1   1       0 1 1 (20.3) Proposition: Let V be a vector space finitely generated over a field F and let f ∈ Bil(V × V ) satisfy the condition that V ⊥f is trivial. Then each subspace W of V satisfies the following conditions: (1) If δ ∈ D(W ) there exists a v ∈ V such that δ(w) = f (v, w) for all w ∈ W ; (2) dim(W ) + dim(W ⊥f ) = dim(V ). Proof: (1) Every vector v ∈ V defines a linear functional δ v ∈ D(V ) by setting δ v : y → f (y, v). Moreover, the function v → δ v from V to D(V ) is a linear transformation, which is a monomorphism as a result of the condition that V ⊥f is trivial. But dim(V ) = dim(D(V )) since V is finitely generated, and hence this is an isomorphism. Now let δ ∈ D(W ) and let Y be a complement of W in V. Then the function from V to F given by w + y → δ(w) belongs to D(V ) and so there exists a vector v ∈ V such that it equals δ v . In particular, δ(w) = f (v, w) for all w ∈ W, proving (1). (2) The function from V to D(W ) which assigns to each v ∈ V the restriction of δ v to W is a linear transformation which, by (1), is an epimorphism. The kernel of this epimorphism consists of all vectors v ∈ V satisfying f (w, v) = 0 for all w ∈ W, and that is precisely W ⊥f . Therefore, by Proposition 6.10, we have (2). In particular, we see from Proposition 20.3, that a necessary and sufficient condition for us to have V = W ⊕ W ⊥f is that W and W ⊥f be disjoint. (20.4) Proposition: Let V and W be vector spaces finitely generated over a field F and let f ∈ Bil(V ×W ) be a bilinear form


405

which is not the 0-function. Then there exist bases {v1 , . . . , vk } and {w1 , . . . , wn } of V and W respectively and there exists a positive integer 1 ≤ t ≤ min{k, n} such that

1 if i = j ≤ t . f (vi , wj ) = 0 otherwise Proof: Since f is not the 0-function, there exist vectors v1 ∈ V and y1 ∈ W such that f (v1 , y1 ) = 0. Therefore, if we set w1 = f (v1 , y1 )−1 y1 , we have f (v1 , w1 ) = 1. Let V1 = F v1 and W1 = F w1 . If we set / W2 W2 = {w ∈ W | f (v1 , w) = 0}, then W1 ∩ W2 = {0W } since cw1 ∈ for all 0 = c ∈ F. We claim that W = W1 ⊕ W2 . Indeed, if w ∈ W and if c = f (v1 , w) then we see that f (v1 , w − cw1 ) = f (v1 , w) − cf (v1 , w1 ) = c − c = 0 and so w − cw1 ∈ W2 , which proves the claim. In a similar way, we have V = V1 ⊕ V2 , where V2 = {v ∈ V | f (v, w1 ) = 0}. Thus we see that f (v, w) = 0 whenever (v, w) ∈ [V1 × W2 ] ∪ [V2 × W1 ]. By passing to the oppose form if necessary, we can assume without loss of generality that k ≤ n. If k = 1, we choose {v1 } as a basis for V and {w1 , . . . , wn } as a basis for W, where {w2 , . . . , wn } is an arbitrary basis for W2 . This proves the proposition, with t = 1. Now assume that k > 1 (which implies n > 1) and that the proposition has been proven whenever dim(V ) < k. In particular, we will look at the restriction of f to V2 × W2 . By the induction hypothesis, there exist bases {v2 , . . . , vk } of V2 and {w2 , . . . , wn } of W2 such that

1 if 2 ≤ i = j ≤ t f (vi , wj ) = . 0 otherwise Then {v1 , . . . , vk } and {w1 , . . . , wn } are the bases we want.

We see that if V and W are vector spaces finitely generated over a field F and if f ∈ Bil(V × W ), then Proposition 20.4 says that there exist bases of V and W with respect to which f is represented by a ! I O matrix of the form . O O We will be particularly interested in symmetric bilinear forms. As an immediate consequence of the definition, we see that if V is a vector space finitely generated over a field F and if B is a given basis for V, then a bilinear form f ∈ Bil(V × V ) is symmetric if and only if the matrix TBB (f ) is symmetric. Moreover, every symmetric matrix is TBB (f ) for some symmetric bilinear form f ∈ Bil(V × V ).

406




Example:

Let 

B

be the canonical basis of

R3

and let

A =

1 −5 3  −5 1 7  . Then A = TBB (f ), where f ∈ Bil(R3 × R3 ) is 3 7 4 defined by     a1 b1 f   a2  ,  b2  a3 b3

=

a1 b1 + a2 b2 − 5(a1 b2 + a2 b1 ) +3(a1 b3 + a3 b1 ) + 7(a2 b3 + a3 b2 ) + 4a3 b3 .

(20.5) Proposition: Let F be a set of characteristic other than 2 and let V be a vector space finitely-generated over F. Let f ∈ Bil(V × V ) be symmetric. Then there exists a basis B = {v1 , . . . , vn } of V such that TBB (f ) is a diagonal matrix.

Proof: The proposition is trivially true if f is the 0-function, and so we can assume that that is not the case. We will proceed by induction on n = dim(V ). For n = 1, the result is again immediate, and so we can assume that n > 1 and that the result has been established for all spaces having dimension less than n. We first claim is that there exists a vector v ∈ V satisfying f (v, v) = 0. Indeed, assume that this is not the case. Then if v and w are arbitrary vectors in V we have 0 = f (v + w, v + w) = f (v, v) + 2f (v, w) + f (w, w) = 2f (v, w) and since the characteristic of F is not 2, this implies that f (v, w) = 0, contradicting our assumption that f is not the 0-function. Hence we can select a vector v1 ∈ V satisfying f (v1 , v1 ) = 0. ⊥ Let V1 = F v1 and let V2 = V1 f . From the definition of V1 it is clear that V1 and V2 are disjoint, and from Proposition 20.3 it follows that V = V1 ⊕ V2 . In particular, dim(V2 ) = n − 1 and so, by the induction hypothesis, there exists a basis C = {v2 , . . . , vn } of V2 , such that, if f2 is the restriction of f to V2 , then TCC (f2 ) is a diagonal matrix. Since f (v1 , vi ) = 0 for all 2 ≤ i ≤ n, it follows that B = {v1 , . . . , vn } does indeed give us the desired result. Thus we see that every symmetric matrix over a field of characteristic other than 2 is congruent to a diagonal matrix. (20.6) Proposition: Let V be a vector space finitely-generated over C and let f ∈ Bil(V × V ) be a symmetric bilinear form of


407

rank r. Then there exists a basis B = {v1 , . . . , vn } of V satisfying the following conditions: (1) TBB (f ) is a diagonal matrix; 1 if 1 ≤ i ≤ r (2) f (vi , vi ) = . 0 otherwise Proof: By Proposition 20.5, we know that there is a basis B = {v1 , . . . , vn } of V satisfying the condition that TBB (f ) is a diagonal matrix. This matrix is of rank r and so, renumbering the basis elements if necessary, we can assume that f (vi , vi ) = 0 when and only when 1 ≤ i ≤ r. For each 1 ≤ i ≤ r, define ci = f (vi , vi )−1/2 ∈ C, and replace vi by ci vi to get a basis satisfying (2) as well. Let V be a vector space finitely-generated over a field F of characteristic other than 2 and let f ∈ Bil(V × V ) be a bilinear form. The function q : V → F defined by q : v → f (v, v) is called the quadratic form defined by f. Note that if a ∈ F and v ∈ V then q(av) = f (av, av) = a2 f (v, v) = a2 q(v). Moreover, if f ∈ Bil(V × V ) and if g ∈ Bil(V × V ) is the symmetric bilinear form given by g : (v, w) →

1 2

[f (v, w) + f (w, v)]

then the quadratic forms defined by f and g are the same. Therefore, without loss of generality, we will always assume that all quadratic forms over such fields are defined by symmetric bilinear forms. We further see that different symmetric bilinear forms define different quadratic forms, since, for any v, w ∈ V, we have f (v, w) = 12 [q(v + w) − q(v) − q(w)] . The classification of quadratic forms is of great importance in analytic geometry and in number theory.1 Example: If V is an inner product space over R, then we have already noted that the function f : (v, w) → v, w is a symmetric bilinear form. 2 The quadratic form defined by f is given by v → v .

1 The theory of quadratic forms over R was developed by Gauss and his student Eisenstein, and the need to study such forms was one of the factors which led to the development of determinant theory. Their work was extended to quadratic forms over C by the 19th-century British mathematician Henry Smith. The fundamental development in the theory of symmetric bilinear forms on vector spaces over fields of characteristic other than 2 is due to the 20th-century German mathematician Ernst Witt.

408


Example: If V is the vector space of all polynomial functions from R to itself, then we have 4 1 a symmetric bilinear form from V × V to R defined by (f, g) → 0 f (t)g(t)dt, which in turn defines the quadratic 41 form f → 0 f (t)2 dt. Example: Let V = bilinear form defined by    a1  a2       a3  ,  a4

R4 and let f ∈ Bil(V × V ) be the symmetric  b1  b2   → a1 b1 + a2 b2 + a3 b3 − a4 b4 ,  b3  b4

which lies at the center of Minkowski’s mathematical formulation of Einstein’s relativity theory. The quadratic form defined by this bilinear form   a1  a2  2 2 2 2  is   a3  → a1 + a2 + a3 − a4 . A similar symmetric bilinear form is a4     a1 b1  a2   b2  2     the Lorentz2 form   a3  ,  b3  → a1 b1 + a2 b2 + a3 b3 − c a4 b4 , a4 b4 where c is the speed of light. The quadratic form defined by this bilinear   a1  a2  2 2 2 2 2  form is   a3  → a1 + a2 + a3 − c a4 . a4 A more general result, also based on the work of Lorentz and Minkowski, gives a fascinating “reversal” of the Cauchy-Schwarz-Bunyakovski inequality. Let n be a positive integer and consider the subset ! (not subspace) a , where a is a U of Rn+1 consisting of all vectors of the form v ! a n nonnegative real number and v ∈ R satisfies v ≤ a. For u = v

2 Dutch physicist Hendrick Antoon Lorentz, the first to conceive of the notion of the electron, won a Nobel prize in 1902. His work formed a basis for much of Einstein’s theory.


409

! b in U, let us define u y to be ab − v · w. By our w assumption on U, we u u ≥ 0 for every u ∈ U. Then one can *√note at + (√ ) show that u y ≥ uu y y . This inequality is often known as the lightcone inequality, because of its applications in physics. and y =

By Proposition 20.6 we see that if V is a vector space finitely generated over C and if f ∈ Bil(V × V ) is symmetric and has rank r, we can find , vn } of V such that the quadratic form q defined by f a basis {v1 , . . . n r is given by q : i=1 ai vi → i=1 a2i . Example: Let F be either R or C. Let n be a positive integer and let A ∈ Mn×n (F ) be symmetric. Let f ∈ Bil(F n , F n ) be the symmetric bilinear form given by f : (v, w) = v T Aw, and let q be the quadratic form defined by f. The set {q(v) | v = 1} (here the norm is the one defined by the dot product on F n ) is called the numerical range of the matrix A. In the case F = C, this is always a bounded convex subset which contains all of the eigenvalues of A. For the special case n = 2, this set is an ellipse with its foci at the eigenvalues of A, assuming that they are distinct, or a circle with center at the sole eigenvalue of A, assuming that A has only one eigenvalue of multiplicity 2. For n > 2, the characterization of the numerical range is much more complicated. (20.7) Proposition: Let n be a positive integer and let A ∈ Mn×n (R) be symmetric. Let f ∈ Bil(Rn × Rn ) be the symmetric bilinear form given by f : (v, w) = v T Aw, and let q be the quadratic form defined by f. Let c1 ≥ c2 ≥ . . . ≥ cn be the eigenvalues of A. Then the numerical range of A lies in the closed interval [cn , c1 ]. Moreover, both endpoints of this interval belong to the numerical range of A. Proof: By Proposition 17.7, we know that there exists an orthonormal basis B = {v1 , . . . , vn } of V consisting of eigenvectors of A. Moreover, if n 2 v ∈ V then v = i=1 v, vi vi by Proposition 17.9, and so 1 = v = n n 2 v, v = i=1 v, vi . We also see that Av = i=1 v, vi A(vi ) = n n 2 T i=1 ci v, vi vi . Thus v Av = v, Av = i=1 ci v, vi . Since " n # " n # n 2 2 2 ≥ = cn . v, vi ci v, vi ≥ cn v, vi c1 = c1 i=1

i=1

i=1

Therefore the numerical range of A lies in the closed interval [cn , c1 ]. If v is a normal eigenvector of A corresponding to cn , then v T Av = v, Av = v, cn v = cn v, v = cn , and similarly for the case of an eigen vector of A satisfying v = 1 and corresponding to c1 .

410


In order to see the geometric significance of quadratic forms, let us recall that a general quadratic equation in three unknowns over R is one of the form a11 X12 + a22 X22 + a33 X32 + 2 (a12 X1 X2 + a13 X1 X3 + a23 X2 X3 ) +b1 X1 + b2 X2 + b3 X3 + c = 0 in which not all of the aij are equal to 0. Such an equation can be written in the form f (v, v) + w · v + c = 0, where f ∈ Bil(R3 , R3 ) is the symmetric bilinear form defined with respect to the canonical basis by     b1 a11 a12 a13 the matrix A =  a12 a22 a23  , where w =  b2  , and where a13 a23 a22 b3   X1 v =  X2  . The graph of such an equation is a quadratic surface. X3 The various quadratic surfaces in R3 can then be classified by considering congruence classes of the matrices A, a task very important in analytic geometry. We will now return to the general case of bilinear transformations. Let F be a field, let V and W be vector spaces over F, and let G = F (V ×W ) . Then G is a subspace of F V ×W having a basis {gv,w | (v, w) ∈ V × W }, where

1 if (v , w ) = (v, w) gv,w : (v , w ) → . 0 otherwise Let H be the subspace of G generated by all functions of the form gv1 +v2 ,w − gv1 ,w − gv2 ,w , gv,w1 +w2 − gv,w1 − gv,w2 , gav,w − agv,w , or gv,aw − agv,w for all v, v1 , v2 ∈ V, w, w1 , w2 ∈ W, and a ∈ F. Let us pick a complement of H in G, and call it V ⊗ W. By Proposition 7.8, we know that V ⊗ W is unique up to isomorphism. Let α be the projection of G with image V ⊗ W coming from the decomposition G = H ⊕ (V ⊗ W ) and, for all v ∈ V and w ∈ W, denote α(gv,w ) by v ⊗ w. Then B = {v⊗w | (v, w) ∈ V ×W } is a generating set for V ⊗W. It is important to emphasize that the elements of V ⊗ W are linear combinations of elements of B. In quantum physics, elements of V ⊗ W B, for suitable spaces V and W, are known as entangled tensors and these have important physical interpretations. Elements of B are known as simple tensors. If v1 , v2 ∈ V and w ∈ W, then [v1 + v2 ] ⊗ w − (v1 ⊗ w) − (v2 ⊗ w) = α (gv1 +v2 ,w − gv1 ,w − gv2 ,w ) = 0G


411

and so [v1 + v2 ] ⊗ w = (v1 ⊗ w) + (v2 ⊗ w) . Similarly, if v ∈ V and w1 , w2 ∈ W then v ⊗ [w1 + w2 ] = v ⊗ w1 + v ⊗ w2 . We also see that if v ∈ V, w ∈ W and c ∈ F, then cv ⊗ w = c(v ⊗ w) = v ⊗ cw. The vector space V ⊗ W is called the tensor product3 of V and W. From the definition of the tensor product, we see that the function tV W from V × W to V ⊗ W given by (v, w) → v ⊗ w is a bilinear transformation. This transformation has a very special significance, due to the following theorem, which allows us to move from bilinear transformations to linear transformations. (20.8) Proposition: Let V, W, and Y be vector spaces over a field F. For each bilinear transformation f ∈ Bil(V × W, Y ) there exists a unique linear transformation α ∈ Hom(V ⊗ W, Y ) satisfying f = αtV W .

Proof: Given f ∈ Bil(V × W, Y ), there exists a linear transformation β ∈ Hom(G, Y ) defined on the elements of a basis of the space G defined above, given by the condition that β : gv,w → f (v, w). Since f is a bilinear transformation, H ⊆ ker(β) and so we can define the linear transformation α ∈ Hom(V ⊗ W, Y ) by setting α:

n

ai [vi ⊗ wi ] →

i=1

n

ai f (vi , wi ).

i=1

n n This function is well-defined since if i=1 ai [vi ⊗ wi ] = i=1 bi [vi ⊗ wi ] n (a − b )g ∈ H ⊆ ker(β). Therefore in V ⊗ W then i vi ,wi i=1 i α

" n i=1

# ai [vi ⊗ wi ]

=α

" n

# bi [vi ⊗ wi ]

i=1

Clearly α is a linear transformation and satisfies f = αtV W .

3

There are many equivalent definitions of the tensor product. The definition given here is due to the 20th-century French mathematician, Claude Chevalley. The notion of a tensor was first introduced in differential calculus by the 19th-century Italian mathematicians Gregorio Ricci-Curbastro and Tullio Levi-Civita and became a central tool in relativity theory.

412


We are left to prove uniqueness. Suppose that γ ∈ Hom(V ⊗ W, Y ) satisfies f = γtV W . In particular, α(v ⊗ w) = γ(v ⊗ w) for all (v, w) ∈ V × W. That is to say, α and γ act identically on a generating set for V ⊗ W and so, in particular, on a basis for V ⊗ W contained in this generating set. Therefore, by Proposition 6.2, it follows that α = γ. The following proposition is very important, and is often used as a basis for the definition of the tensor product. (20.9) Proposition: If V, W, and Y are vector spaces over a field F then the vector spaces Hom(V ⊗ W, Y ) and Hom(V, Hom(W, Y )) are isomorphic. Proof: It is easy to see that the function Hom(V ⊗ W, Y ) → Bil(V × W, Y ) defined by β → βtV W is a linear transformation and from Proposition 20.8 it follows that this is an isomorphism. Therefore the result follows from Proposition 20.1. Example: Let V and W be vector spaces over a field F and let δ 1 ∈ D(V ) and δ 2 ∈ D(W ) be linear functionals. Then there exists a bilinear form in Bil(V × W ) defined by (v, w) → δ 1 (v)δ 2 (w). From Proposition 20.8, it follows that there functional δ 1 ⊗ δ 2 ∈ n exists a linear n D(V ⊗ W ) satisfying δ 1 ⊗ δ 2 : i=1 ai [vi ⊗ wi ] → i=1 ai δ 1 (vi )δ 2 (wi ). Example: More generally, let V and W be vector spaces over a field F , let α be an endomorphism of V, and let β be an endomorphism of W. The function from V × W to V ⊗ W defined by (v, w) → α(v) ⊗ β(w) is a bilinear transformationand so defines an endomorphism α ⊗ β of n n V ⊗ W satisfying α ⊗ β : i=1 ai [vi ⊗ wi ] → i=1 ai [α(vi ) ⊗ β(wi )] . By Proposition 5.13, we know that if V ⊕ W is a vector space finitelygenerated over a field F, then dim(V ⊕ W ) = dim(V ) + dim(W ). We now prove the “multiplicative” analog of this assertion for tensor products. (20.10) Proposition: Let V and W be vector spaces finitely generated over a field F. Then V ⊗ W is also finitely generated, and dim(V ⊗ W ) = dim(V ) dim(W ). Proof: Let us choose bases {v1 , . . . , vk } of V and {w1 , . . . , wn } n k and w = of W. Then for any v = i=1 ai vi ∈ V j=1 bj wj ∈


413

k n W, we see that v ⊗ w = i=1 j=1 ai bj (vi ⊗ wj ). Thus we see that {vi ⊗ wj | 1 ≤ i ≤ k and 1 ≤ j ≤ n} is a generating set for V ⊗W, showing that V ⊗ W is finitely-generated. Moreover, by Proposition 20.9 and Proposition 14.6, we see that the dimension of V ⊗ W is equal to the dimension of D(V ⊗ W ) and hence to the dimension of Hom(V, D(W )), and this is equal to the dimension of Hom(V, W ), which is precisely dim(V ) dim(W ). In particular, we see that in the context of Proposition 20.10, the set {vi ⊗ wj | 1 ≤ i ≤ k and 1 ≤ j ≤ n} is in fact a basis of V ⊗ W. Example: Let F be a field and let k and n be positive integers. Then, by Proposition 20.10, we know that dim(F k ⊗F n ) = kn = dim(Mk×n (F )), and so the vector spaces F k ⊗F n and Mk×n (F ) are isomorphic. Indeed, if we choose bases {v1 , . . . , vk } of V and {w1 , . . . , wn } of W, then the function vi ⊗ wj → vi ∧ wj extends to an isomorphism between these two spaces.

Example: Let F be a field, let n be a positive integer, and let V be a vector space finitely generated over F and having a basis {v1 , . . . , vk }. The dimension of the vector space Mn×n (V ) over F is n2 k. Consider the bilinear transformation f : Mn×n (F ) × V → Mn×n (V ) defined by ([aij ], v) → [aij v]. By Proposition 20.8, we know that this bilinear transformation defines a linear transformation α : Mn×n (F ) ⊗ V → Mn×n (V ) and it is clear that this is an epimorphism. But, by Proposition 20.10, we see that the dimension of Mn×n (F ) ⊗ V is also equal to n2 k and so α must be an isomorphism. Example: Let F be a field and let k, n, s, and t be positive integers. Let f : Mk×n (F ) × Ms×t (F ) → Mks×nt (F ) be the function defined by   a11 B . . . a1n B   .. f : (A, B) →  ...  . This is a bilinear transformation . ak1 B

...

akn B

of vector spaces over F and so by Proposition 20.8, it defines a linear transformation α : Mk×n (F )⊗Ms×t (F ) → Mks×nt (F ) which, again, can be shown to be an isomorphism. In the literature, it is usual to write A⊗B instead of f (A, B). This matrix is called the Kronecker product of the matrices A and B. Kronecker products are very important in matrix theory and its applications. It is easy to see that for all such matrices A and B we have (A ⊗ B)T = AT ⊗ B T . Moreover, if k = n and s = t and if A and B are nonsingular, then A ⊗ B is nonsingular, and (A ⊗ B)−1 = A−1 ⊗ B −1 . We also note that if A and B are symmetric

414


then so is A ⊗ B. Furthermore, Cholesky or QR-factorizations of A ⊗ B come immediately from the corresponding factorizations of A and B. Let V, V , W and W be vector spaces over a field F. If α ∈ Hom(V, V ) and β ∈ Hom(W, W ) then we have a bilinear transformation V ×W → V ⊗W defined by (v, w) → α(v)⊗β(w) and so, by Proposition 20.8, there exists a linear transformation from V ⊗W to V ⊗W satisfying v ⊗ w → α(v) ⊗ β(w). We will denote this linear transformation by α ⊗ β. (20.11) Proposition: Let V, V , W, and W be vector spaces finitely generated over a field F. Any n element of the space Hom(V ⊗ W, V ⊗ W ) is of the form i=1 αi ⊗ β i , where αi ∈ Hom(V, V ) and β i ∈ Hom(W, W ) for each 1 ≤ i ≤ n. Proof: The function (α, β) → α⊗β from Hom(V, V )×Hom(W, W ) to Hom(V ⊗W, V ⊗W ) is bilinear and so defines a linear transformation ϕ : Hom(V, V ) ⊗ Hom(W, W ) → Hom(V ⊗ W, V ⊗ W ). We are done if we can show that ϕ is an isomorphism. By Propositions 8.1 and 20.10, we know that dim(Hom(V, V ) ⊗ Hom(W, W )) = dim(Hom(V, V )) dim(Hom(W, W )) = dim(V ) dim(V ) dim(W ) dim(W ) = dim(V ⊗ W ) dim(V ⊗ W ) = dim(Hom(V ⊗ W, V ⊗ W ) and so it suffies to provethat ϕ is a monomorphism. n Indeed, assume that i=1 αi ⊗ β i ∈ ker(ϕ), where the set {β 1 , . . . , β n } is linearly independent, and where none of the αi is the 0-function. Then n ⊗W α (v) ⊗ β (w) = 0 for all v ∈ V and all w ∈ W. Pick i V i i=1 v ∈ V satisfying α1 (v) = 0V . By renumbering if necessary, we can assume that {α1 (v), . . . , αk (v)} is a maximal linearly-independent subset of {α1 (v), . . . , αn (v)}. Therefore, for each k < h ≤ n there exists a scalar k bhj , not all of them being equal to 0, such that αh (v) = j=1 bhj αj (v) and so   k m k  αi (v) ⊗ β i (w) + bhj αj (v) ⊗ β h (w) 0V ⊗W =

=

i=1

h=k+1

k

k

αi (v) ⊗ β i (w) +

i=1

=

k i=1

" αi (v) ⊗

αj (v) ⊗

j=1

β i (w) +

j=1

m h=k+1

"

m

# bhj β h (w)

h=k+1

#

bhj β h (w) .


415

Since the {α1 (v), . . . , αk (v)} is linearly independent, we must have set m + h=k+1 bhj β h (w) = 0W for all 1 ≤ i ≤ k and all w ∈ W. Hence β i (w) m β i + h=k+1 bhj β h is the 0-function for all 1 ≤ i ≤ k, contradicting the assumption that the set {β 1 , . . . , β n } is linearly independent. We therefore conclude that ker(ϕ) is trivial, which is what we needed to prove. (20.12) Proposition: If U, V and W are vector spaces over a field F, then U ⊗ (V ⊗ W ) ∼ = (U ⊗ V ) ⊗ W. Proof: The bilinear transformation U × (V ⊗ W ) → (U ⊗ V ) ⊗ W defined by (u, v ⊗ w) → (u ⊗ v) ⊗ w induces a linear transformation α : U ⊗ (V ⊗ W ) → (U ⊗ V ) ⊗ W which satisfies u ⊗ (v ⊗ w) → (u ⊗ v) ⊗ w. Similarly we have a linear transformation β : (U ⊗ V ) ⊗ W → U ⊗ (V ⊗ W ) which satisfies (u ⊗ v) ⊗ w → u ⊗ (v ⊗ w). Since αβ and βα are clearly the respective identity maps, we see that α must be the isomorphism we seek. (20.13) Proposition: If V and W are vector spaces over a field F, then V ⊗ W ∼ = W ⊗ V. Proof: The bilinear transformation V × W → W ⊗ V defined by (v, w) → w ⊗ v induces a linear transformation α from V ⊗ W to W ⊗ V satisfying α : v ⊗ w → w ⊗ v. Similarly, there exists a linear transformation β : W ⊗ V → V ⊗ W satisfying β : w ⊗ v → v ⊗ w. Since αβ and βα are clearly the respective identity maps, we see that α must be the isomorphism we seek. Finally, let us briefly mention two algebras built on the notion of the tensor product. The study of these algebras is beyond the scope of this book. However, the reader should be aware of them and will find it fruitful to explore them further. In what ensues, V is an arbitrary vector space over a field F. (I) For each nonnegative integer k, we define the vector space V ⊗k over F J by setting V ⊗0 = V and V ⊗k = V ⊗(k−1) ⊗ V if k > 0. Let ∞ T (V ) = V ⊗k . We can define a product • on T (V ) by setting k=0

(v1 ⊗ . . . ⊗ vk ) • (vk+1 ⊗ . . . ⊗ vm ) = v1 ⊗ . . . ⊗ vk+m for all v1 , . . . , vk+m ∈ V and extend linearly. This is an F -algebra, known as the tensor algebra of V over F. The tensor algebra has several important properties, one of which is that if K is any algebra over F then any linear transformation α : V → K can be uniquely extended to a homomorphism of F -algebras from T (V ) to K. Moreover, if W is a vector space over F then any linear transformation α : V → W

416


can be uniquely extended to a homomorphism of F -algebras from T (V ) to T (W ). (In the language of category theory, this says that T ( ) is a functor from the category of vector spaces over F to the category of F -algebras.) (II) Let Y be the subspace of V ⊗ V generated by {v ⊗ v | v ∈ V }. Then a complement of Y in V ⊗ V is called an exterior square of V and is denoted by V ∧ V . This space is unique up to isomorphism. If α is the projection of V ⊗ V with image V ∧ V and kernel Y, denote α(v ⊗ w) by v ∧ w. Since (v + w) ⊗ (v + w) = v ⊗ v + v ⊗ w + w ⊗ v + w ⊗ w for all v, w ∈ V, we see that v ∧ w = −w ∧ v for all v, w ∈ V. Therefore, if V is finitely-generated over F with basis {v1 , . . . , vn }, we see that {v i ∧ vj | 1 ≤ i < j ≤ n} is a basis for V ∧ V, and hence dim(V ∧ V ) = n2 = 12 n(n − 1). This construction can be iterated to more than two factors. If k > 0 is an integer, we can consider the subspace Y of V ⊗k generated by all expressions of the form v1 ⊗ . . . ⊗ vk in which vi = vj for some i = j. A complement of Y is denoted by ∧k V and is called the kth exterior power of V. If V has finite dimension n, then dim(∧k V ) = nk . In particular, we note that ∧k V is trivial when Jn ∧k V of T (V ) is known as the k > n. The subspace ∧(V ) = k=0 exterior algebra of V, and has important applications in geometry and cohomology theory. One can show that if (K, •) is a unital F -algebra and if α : V → K is a linear transformation satisfying the condition that α(v) • α(v) = 0K for all v ∈ V, then α can be uniquely extended to a homomorphism of unital F -algebras from ∧(V ) to K.

Exercises

Exercise 1044 Find  1  0 0

a real number a such that the matrices    a a 1 −1 −1 1 a  and  −1 1 −1  0 1 −1 −1 1

define the same bilinear form in Bil(R3 , R3 ). Exercise 1045 Let V = QQ . Is the function from V × V to Q given by (f, g) → (f + g)( 12 )(f − g)(2) a bilinear form?


417

Exercise 1046 Let F be a field and let u : N × N → F be an arbitrary function. Is the function fu : F [X] × F [X] → F [X] defined by     ∞ ∞ ∞  ai X i , bj X j  → u(i, j)ai bj X k  fu :  i=0

j=0

k=0

i+j=k

a bilinear transformation? Exercise 1047 Let B be the canonical basis for the vector space V = R2 . Find a bilinear form f ∈ Bil(V × V ) satisfying the condition TBB (f ) =

2 2 4 −1

! .

Exercise 1048 Let B be the canonical basis for R3 . Find TBB (f ), where f : R3 × R3 → R is the bilinear form defined by    a a f :  b  ,  b  → aa + 2bc + cc + 2cb − ab + bb − ba . c c 

f : R3 × R3 → R be the bilinear form defined by  0 1 0 f : (v, w) → v ·  1 0 2  w. Find the matrix representing f with 0 1 1       0 1   1  0 , 1 , 0  respect to the basis of R3 .   0 1 1 Exercise 1049 Let 

Exercise 1050 Let V and W be vector spaces over a field F and let α ∈ Hom(V, W ). For each g ∈ Bil(W × W ), let us define the bilinear form gα ∈ Bil(V × V ) by setting gα : (v, v ) → g(α(v), α(v )). Is the function g → gα a linear transformation? Exercise 1051 Let F be a field of characteristic other than 2 and let V be a vector space over F. Let f ∈ Bil(V × V ). Show that f (v, v) = 0 for all 0V = v ∈ V if and only if for every nontrivial subspace W of V and for every 0V = w ∈ W there exists a vector w ∈ W satisfying f (w, w ) = 0. Exercise 1052 Show that if V and W are vector spaces finitely generated over a field F of unequal dimensions, then there is no nondegenerate f ∈ Bil(V, W ).

418


Exercise 1053 Let F be a field of characteristic 0 and let the bilinear form f ∈ Bil(F 3 × F 3 ) be defined by    a a f :  b  ,  b  → aa + bb − cc . c c 

Is there a nontrivial subspace W of V w, w ∈ W ? Exercise 1054 Let f  1 0  0 1 where A =   0 0 0 0

satisfying f (w, w ) = 0 for all

∈ Bil(R4 × R4 ) be defined by f : (v, w) → v · (Aw),  0 0 0 0   . Find a basis {v1 , v2 , v3 , v4 } of R4 1 0  0 −1

satisfying the condition that f (vi , vi ) = 0 for all 1 ≤ i ≤ 4. Exercise 1055 Let f : Mn×n (F ) × Mn×n (F ) → F be the function defined by f : (A, B) → tr(AB), where F is a field and n is a positive integer. Is f a bilinear form? Exercise 1056 Let n be a positive integer and let f : Mn×n (C) × Mn×n (C) → C be the function defined by f : (A, B) → n · tr(AB) − tr(A)tr(B). Show that f is a symmetric bilinear form. Exercise 1057 Let V be a vector space over a field F and let f ∈ Bil(V, V ) be a symmetric bilinear form. Let Y = F × V and define an operation • on Y by setting (a, v) • (b, w) = (ab + f (v, w), aw + bv) for all a, b ∈ F and all v, w ∈ V. Show that (Y, •) is a Jordan algebra. Exercise 1058 Let V be a vector space over Q. Is the function V ×V → V defined by (v, v ) → v + v a bilinear transformation?     25 −5 35 0 0 0 1  0 −3 21  Exercise 1059 Are the matrices  1 1 0  and 25 0 −4 28 1 1 1 in M3×3 (R) congruent? Exercise 1060 Find an upper-triangular matrix in M3×3 (R) congruent   1 0 −2 1 0  or show that there is no such matrix. to  −1 0 −2 4


419

Exercise 1061 Let F be a field and let n be a positive integer. A matrix A = [aij ] ∈ Mn×n (F ) is an upper Hessenberg matrix if and only if aij = 0 whenever i − j ≥ 2. Is every matrix in Mn×n (R) necessarily congruent to an upper Hessenberg matrix? Exercise 1062 Let F be a field. Show that every upper triangular matrix in M3×3 (F ) is congruent to a lower triangular matrix. Exercise 1063 Let n be a positive integer and let A be a nonsingular symmetric matrix in Mn×n (C). Show that A is congruent to A−1 . Exercise  2 1 P 1 0 3 1

1064  Find a matrix P ∈ M3×3 (R) 3 1  P T is diagonal. 3 

1  1 Exercise 1065 Let A =   1 1

1 1 1 1

1 1 1 1

such that the matrix

 1 1   ∈ M4×4 (R). Find a nonsin1  1

gular matrix P ∈ M4×4 (R) such that P AP T is diagonal. Exercise 1066 Find a diagonal matrix in M4×4 (R) congruent to the   1 2 3 2  2 3 5 8   matrix   3 5 8 10  . 2 8 10 −8 

 1 i 1+i 0 2 − i  ∈ M3×3 (C) conExercise 1067 Is the matrix  i 1 + i 2 − i 10 + 2i gruent to I? Exercise 1068 Let n be a positive integer and let α be a positive-definite endomorphism of Rn represented with respect to the canonical basis by the matrix A. If A is a matrix congruent to A, does it too represent a positive-definite endomorphism of Rn with respect to the canonical basis? Exercise 1069 Let V be a vector space finitely generated over be a field F of characteristic other than 2. If f ∈ Bil(V, V ) is symmetric and not the 0-function, show that there exists a vector v ∈ V satisfying f (v, v) = 0. Exercise 1070 Let V be a vector space finitely generated over be a field F of characteristic other than 2. If f ∈ Bil(V, V ), show that f (v, v) = 0 for all v ∈ V if and only if f (v, w) = −f (w, v) for all v, w ∈ V.

420


Exercise 1071 Let n be a positive integer, let F be a field, and let A ∈ Mn×n (F ). Show that there exists a symmetric matrix B ∈ Mn×n (F ) satisfying v · Av = v · Bv for all v ∈ F n . Exercise 1072 Find a bilinear form f ∈ Bil(R3 , R3 ) which defines the   a quadratic form  b  → a2 − 2ab + 4ac − 2bc + 2c2 . c Exercise 1073 Let f ∈ Bil(R3 , R3 ) be the symmetric bilinear form de  −3 1 0 fined by the matrix  1 −6 1  . Find the quadratic form defined by 0 1 7 f. Exercise 1074 Let f ∈ Bil(R3 , R3 ) be the symmetric bilinear form de  2 −1 5 1  0 fined by the matrix  −1 . Find the quadratic form defined 3 1 5 −3 3 by f. Exercise 1075 Find a symmetric bilinear form f ∈ Bil(R3 , R3 ) which   a defines the quadratic form  b  → 2ab + 4ac + 6bc. c Exercise 1076 Let F be a field of characteristic other than 2, and let V be a vector space over F. Let q : V → F be a function satisfying the condition that q(v + w) + q(v − w) = 2q(v) + 2q(w) for all v, w ∈ V. Show that the function f : V × V → F defined by f : (v, w) →

1 4

[q(v + w) − q(v − w)]

is a symmetric bilinear form. Exercise 1077 Let V be a vector space over a field F of characteristic other than 2, and let f ∈ Bil(V, V ) be a symmetric bilinear form which defines a quadratic form q : V → F. Show that q(u + v + w) = q(u + v) + q(u + w) + q(v + w) − q(u) − q(v) − q(w) for all u, v, w ∈ V. Exercise 1078 Find the numerical range of the quadratic form q : R2 → ! 1 0 v. R defined by q : v −→ v T 0 0


Exercise 1079 Let V ∼ = F ⊗ V.

V

be a vector space over a field

F.

421

Show that

Exercise 1080 Let V and W be vector n spaces over a field F. Let x ∈ V ⊗ W be written in the form x = i=1 vi ⊗ wi , where n is minimal k in the sense that there is no way to express x in the form i=1 vi ⊗ wi for any k < n. Show that {v1 , . . . vn } is a linearly-independent subset of V and that {w1 , . . . wn } is a linearly-independent subset of W. Exercise 1081 Let K be a field containing F as a subfield. If V is a vector space over F, show that K ⊗ V is a vector space over K. Exercise 1082 Let V be a vector space of finite dimension n over a field F and let Y be the subspace of V ⊗ V generated by all elements of the form v ⊗ v − v ⊗ v, where v, v ∈ V. Find the dimension of Y. Exercise 1083 Let V and W be finite dimensional vector spaces over a field F . Let v, v ∈ V and w, w ∈ W be vectors satisfying the condition v ⊗ w = v ⊗ w and this is not the identity element of V ⊗ W with respect to addition. Show that there exists a scalar c ∈ F such that v = cv and w = cw. Exercise 1084 Let F be a field and, for all A, B ∈ M2×2 (F ), denote the Kronecker product of A and B by A ⊗ B. If {H1 , . . . , H4 } is the canonical basis for M2×2 (F ), is {Hi ⊗ Hj | 1 ≤ i, j ≤ 4} a basis for M4×4 (F ). Exercise 1085 Let n be a positive integer and let F be a field. If A ∈ Mn×n (F ) is a magic matrix, is the same true for A ⊗ A ∈ M2n×2n (F )? Exercise 1086 Let F be a field and let k and n be positive integers. If matrices A ∈ Mk×k (F ) and B ∈ Mn×n (F ) have eigenvalues a and b respectively, show that ab is an eigenvalue of A ⊗ B. Exercise 1087 Let F be a field and let k and n be positive integers. If matrices A ∈ Mk×k (F ) and B ∈ Mn×n (F ) have eigenvalues a and b respectively, find a matrix C ∈ Mkn×kn (F ) with eigenvalue a + b. Exercise 1088 Let F be a field of characteristic other than 2 and let V be a vector space over F. Find the minimal polynomial of the endomorphism α of V ⊗ V defined by α:

n i=1

ai (vi ⊗ wi ) →

n

ai (wi ⊗ vi ).

i=1

Exercise 1089 Let F be a field, let k, n, s, and t be positive integers, and consider matrices A ∈ Mk×n (F ) and B ∈ Ms×t (F ). Is the rank of A ⊗ B necessarily equal to the product of the ranks of A and B?

422


Exercise 1090 Let V, V , W, W be vector spaces over a field F and let α : V → V and β : W → W be monic linear transformations. Let α ⊗ β be the linear transformation from V ⊗ V to W ⊗ W α⊗β :

n

ai (vi ⊗ vi ) →

i=1

n

ai [α(vi ) ⊗ β(vi )] .

i=1

Is α ⊗ β necessarily monic? Exercise 1091 Let F be a field and let (K, •) and (L, ∗) be F -algebras. Define an operation on V ⊗ W by setting (v ⊗ w) (v ⊗ w ) = (v • v ) ⊗ (w ∗ w ). for all v.v ∈ K and w, w ∈ L. Is (K ⊗ L, ) an F -algebra? Exercise 1092 Let V = R2 and let W = V ⊗ V. If w ∈ W is normal, do there necessarily exist normal vectors v, v ∈ V such that w = v ⊗ v ? Exercise 1093 Let V be an inner product space over R having a basis {vi | i ∈ Ω} and let W be an inner product space over R having a basis {wj | j ∈ Λ} Define a function µ : (V ⊗ W ) × (V ⊗ W ) → R by setting   µ :  aij (vi ⊗ wj ), bij (vi ⊗ wj ) → i∈Ω j∈Λ

i∈Ω j∈Λ

( F) E aij bij vi , vi + wj , wj .

i∈Ω j∈Λ

Is µ an inner product on V ⊗ W ? Exercise 1094 Let V be a vector space over a field F End(V ). Is the function V ∧ V → V ∧ V defined by n

ci (vi ∧ wi ) →

i=1

a linear transformation?

n i=1

ci (α(vi ) ∧ α(wi ))

and let α ∈

Appendix A Summary of Notation

Re(z), 7 im(z), 7 z, 8 √ Q( p), 9 Z/(p), 9 GF (p), 9 i∈Ω Vi , 19 Mk×n (V ), 20 V Ω , 19 χ B , 21 i∈Ω Vi , 22 (Ω) V , 22 F v, 23 F D, 24 i∈Ω Wi , 27 K − , 36 v × w, 36 K + , 37 deg(f ), 38 F [X], 38 F [g(X)], 38 Φq (X), 42 423

424

Appendix A. Summary of Notation

µ(d), 42 F [X1 , . . . , Xn ], 44 dim(V ), 64 U ,⊕ W, 66 i∈Ω Wi , 67 gr(f ), 81 Hom(V, W ), 82 ker(α), 84 im(α), 85 AT , 85 Af f (V, W ), 87 ∼ =, 87 rk(α), 89 null(α), 89 V /W, 98 End(V ), 99 σ c , 99 Aut(V ), 101 εhk , 102 εh;c , 102 εhk;c , 102 ΦBD , 118 v w, 121 v ∧ w, 121 Ehk , 137 Eh;c , 137 Ehk;c , 137 Sn , 202 sgn(π), 203 |A|, 203 adj(A), 213 spec(α), 229 ρ(A), 233 comp(p), 240 A ∼ B, 241 Ann(v), 247 mA (X), 248 F [α]v0 , 267 LR(V ), 268 D(V ), 285 tr(A), 286 v, w , 300 v · w, 300 DH , 301 v , 305

Appendix A. Summary of Notation

eA , 316 cos(A), 15 sin(A), 15 v ⊥ w, 326 W ⊥ , 330 α∗ , 339 Rα , 354 SO(n), 375 √ α, 381 α+ , 390 Bil(V × W, Y ), 399 f op , 399 Bil(V × W ), 401 TBD (f ), 402 v ⊥f w, 403 A⊥f , 403 q(v), 407 V ⊗ W, 410 v ⊗ w, 410 A ⊗ B, 413 V ∧ V, 416 V ⊗k , 415 ∧k V, 416 ∧(V ), 416

425

Index

addition in a field, 6 vector, 17 adjacency matrix, 353 adjoint matrix, 213 adjoint transformation, 339 affine subset, 86 affine transformation, 86 algebra, 33 anticommutative, 34 associative, 33 Cayley, 302 commutative, 34 division, 45 entire, 38 exterior, 416 Jordan, 37 Lie, 35 optimization, 10 quaternion, 58 tensor, 415 unital, 33 algebraic, 65 algebraic multiplicity, 244 algebraically closed, 43

alphabet, 20 angle, 325 annihilate, 247 anti-Hermitian matrix, 366 anticommutative algebra, 34 antitrace, 296 Apollonius’ identity, 323 Arnoldi process, 331 associative algebra, 33 automorphism, 101 elementary, 102 of algebras, 101 unitary, 369 Axiom of Choice, 3 band matrix, 133 basis, 55 canonical, 57, 271 dual, 290 Hamel, 61 Bernstein function, 94 Bessel’s identity, 336 best approximation, 395 bijective, 2 bilinear form, 401 427

428

Index

nondegenerate, 401 bilinear transformation, 399 symmetric, 399 Binet-Cauchy identity, 322 binomial formula, 16 block form, 123 bounded, 60, 307 bounded support, 347 bra-ket product, 121 Brauer’s Theorem, 314 canonical basis, 57, 271 Cantor set, 61 cartesian product, 2 Cassini oval, 314 Cauchy-Schwarz-Bunyakovsky Theorem, 304 Cayley algebra, 302 Cayley-Hamilton Theorem, 250 chain, 53 chain subset, 53 change-of-basis matrix, 146 characteristic, 10 characteristic function, 21 characteristic polynomial, 239, 268 characteristic value, 229 characteristic vector, 229 Chebyshev polynomial, 327 Cholesky decomposition, 360 circulant matrix, 156 co-independent hyperplanes, 298 coefficient, 38 Fourier, 333 leading, 38 Taylor, 104 coefficient matrix, 171 column equivalent, 145 column space, 179 combination linear, 24 commutative algebra, 34 commuting pair, 36 companion matrix, 240 complement, 68 orthogonal, 330

completely reducible, 43 complex conjugate, 8 complex number, 7 condition number, 190 spectral, 383 congruent matrices, 403 conjugate transpose, 301 conjugate, complex, 8 continuant, 221 convex subset, 365 coproduct direct, 22 Courant-Fischer Minimax Theorem, 354 Cramer’s Theorem, 215 cross product, 36 Crout’s algorithm, 153 cyclic, 104 cyclotomic polynomial, 42 decomposition Cholesky, 360 direct sum, 67 LU, 153 polar, 382 QR, 335 singular value, 382 spectral, 379 defective eigenvalue, 244 degree of a generalized eigenvector, 275 of a polynomial, 38 of a polynomial function, 41 derivation, 100 derogatory endomorphism, 244 determinant, 205 determinant function, 199 diagonal matrix, 132 diagonalizable endomorphism, 236 difference set, 2 differential, 80 differential operator, 100 dimension, 63

Index

Dirac functional, 289 direct coproduct, 22 direct product, 19 direct sum, 66 direct sum decomposition, 67 discrete cosine transform, 137 discrete Fourier transform, 136, 308 disjoint subspaces, 23 distance, 315 distribution, 286 division algebra, 45 Division Algorithm, 40 domain, 2 integral, 10 dot product, 300 weighted, 301 dual basis, 290 dual space, 285 weak, 290 dyadic product, 130 eigenspace, 231, 233 generalized, 276 eigenvalue, 229, 232 defective, 244 semisimple, 244 simple, 244 eigenvector, 229, 232 generalized, 275 Eisenstein’s criterion, 42 elementary automorphism, 102 elementary matrix, 137 elementary operation, 143 endomorphism, 99 bounded, 112 derogatory, 244 diagonalizable, 236 nilpotent, 272 normal, 375 orthogonally diagonalizable, 352 positive definite, 356 selfadjoint, 349 entangled tensors, 410 entire, 38

429

epic, 2 epimorphism, 85 equal functions, 2 equivalence relation, 106 equivalent matrices, 145 euclidean norm, 305 subfield, 299 evaluation functional, 291 even function, 69 even permutation, 203 Exchange Property, 26 extended coefficient matrix, 171 exterior algebra, 416 exterior power, 416 exterior product, 121 exterior square, 416 factor space, 98 fan, 168 fast Fourier transform, 136 Fibonacci sequence, 269 field, 6 algebraically closed, 43 formally-real, 300 Galois, 9 orderable, 16 field of algebraic numbers, 65 finite dimensional, 63 finitely generated, 26 fixed point, 231 fixed space, 231 form bilinear, 401 Lorentz, 408 quadratic, 407 formal differentiation, 104 formally real field, 300 Fourier coefficient, 333 Fredholm alternative, 293 Frobenius norm, 311 full pivoting, 152 function, 2 characteristic, 21 determinant, 199

430

Index

even, 69 inverse, 2 odd, 69 periodic, 62 piecewise constant, 30 spline, 48 functional Dirac, 289 evaluation, 291 linear, 285 zero, 285 Fundamental Theorem of Algebra, 43 Galois field, 9 Gauss-Jordan method, 175 Gauss-Seidel iteration method, 186 Gaussian elimination, 175 general Lie algebra, 131 general quadratic equation, 410 generalized eigenspace, 276 generalized eigenvector, 275 generating set, 25 geometric multiplicity, 244 Gershgorin bound, 312 Gershgorin’s Theorem, 312 Givens rotation matrix, 370 GMRES algorithm, 331 golden ratio, 269 Google matrix, 254 Gram matrix, 303 Gram-Schmidt process, 328 Gram-Schmidt Theorem, 328 graph, 81 Grassmann’s Theorem, 69 Greville’s method, 392 group of automorphisms, 107 Guttman’s Theorem, 138 Haar wavelet, 332 Hadamard inequality, 329 Hadamard matrix, 207 Hadamard product, 157 Hamel basis, 61 Hamming norm, 315

Hankel matrix, 219 Hausdorff Maximum Principle, 60 Hermitian matrix, 351 Hermitian transpose, 301 Hibert subset, 332 Hilbert matrix, 144 Hilbert-Schmidt norm, 311 homogeneous system of linear equations, 170 homomorphism, 79 of algebras, 79 of unital algebras, 79 Householder matrix, 373 hyperplane, 292 ill-conditioned, 189 image, 85 imaginary part, 7 improper subspace, 22 independent subspaces, 67 indeterminate, 38 index of nilpotence, 272 induced norm, 310 infinite dimensional, 63 inner product, 299 inner product space, 300 integral domain, 10 interior product, 121 interpolation problem, 169 intersection, 2 invariant subspace, 103 inverse function, 2 inversion, 202 involution, 341 irreducible, 41 isometry, 362 isomorphic vector spaces, 87 isomorphism, 85 of algebras, 85 of unital algebras, 85 iteration method Gauss-Seidel, 186 Jacobi, 186 Jacobi identity, 36

Index

Jacobi iteration method, 186 Jacobi overrelaxation method, 188 Jacobi polynomial, 327 JOR, 188 Jordan algebra, 37 Jordan canonical form, 275, 278 Jordan identity, 37 Jordan product, 37 Karatsuba’s algorithm, 39 kernel, 84 ket-bra product, 121 Kovarik algorithm, 393 Kronecker product, 413 Krylov algorithm, 271 Krylov subspace, 267 Lagrange identity, 306 Lagrange interpolation polynomial, 146 Lanczos algorithm, 271 leading coefficient, 38 leading entry, 174 least squares method, 395 Legendre polynomial, 326 Lie algebra, 35 general, 131 special, 286 Lie product, 36 lightcone inequality, 409 linear combination, 24 linear functional, 285 linear transformation, 79 adjoint of, 339 linearly dependent, 49 locally, 82 linearly independent, 49 linearly recurrent sequence, 268 list, 1 locally linearly dependent, 82 Loewner partial order, 357 Lorentz form, 408 lower-triangular matrix, 134 LU-decomposition, 153 M¨ obius function, 42

431

magic matrix, 259 Markov matrix, 135 matrices column-equivalent, 145 congruent, 403 equivalent, 145 row-equivalent, 145 similar, 241 unitarily similar, 370 matrix, 20 adjacency, 353 adjoint, 213 anti-Hermitian, 366 band, 133 change-of-basis, 146 circulant, 156 coefficient, 171 companion, 240 determinant of, 205 diagonal, 132 elementary, 137 extended coefficient, 171 Givens rotation, 370 Google, 254 Gram, 303 Hadamard, 207 Hankel, 219 Hermitian, 351 Hilbert, 144 Householder, 373 in block form, 123 in reduced row echelon form, 174 in row echelon form, 173 lower-triangular, 134 magic, 259 Markov, 135 Nievergelt’s, 144 nonsingular, 135 normal, 384 orthogonal, 372 permutation, 142 quasidefinite, 366 scalar, 132 singular, 135

432

Index

skew-symmetric, 134 sparse, 187 special orthogonal, 375 stochastic, 135 symmetric, 134 symmetric Toeplitz, 183 transpose, 85 tridiagonal, 133 unitary, 370 upper Hessenberg, 419 upper-triangular, 133 Vandermonde, 147 zero, 21 maximal, 53 maximal subspace, 292 minimal, 53 minimal polynomial, 248, 268 Minkowski’s inequality, 307 minor, 209 Modular Law, 28 monic function, 2 polynomial, 38 monomorphism, 85 Moore-Penrose pseudoinverse, 389 multiplication in a field, 6 scalar, 17 multiplication table, 58 multiplicity algebraic, 244 geometric, 244 mutually orthogonal, 326 Nievergelt’s matrix, 144 nilpotent, 272 nondegenerate bilinear form, 401 nonhomogeneous system of linear equations, 170 nonsingular matrix, 135 nontrivial subspace, 22 norm, 305, 309 euclidean, 305 Frobenius, 311 Hamming, 315

Hilbert-Schmidt, 311 induced, 310 spectral, 311 normal endomorphism, 375 normal matrix, 384 normal vector, 305 normed space, 309 nullity, 89 number complex, 7 rational, 5 real, 5 numerical range, 409 odd function, 69 odd permutation, 203 operation elementary, 143 opposite transformation, 399 optimization algebra, 10 order of recurrence, 268 orderable field, 16 orthogonal, 326 orthogonal complement, 330 right, 403 orthogonal matrix, 372 orthogonal projection, 330 orthogonality with respect to a bilinear form, 403 orthogonally diagonalizable, 352 orthonormal, 331 Padé approximant, 216 pairwise disjoint, 24 Parallelogram law, 307 parity, 401 Parseval’s identity, 336 partial order, 53 Loewner, 357 partial pivoting, 152 partially-ordered set, 53 periodic function, 62 permutation, 2 even, 203 odd, 203

Index

permutation matrix, 142 Pfaffian, 206 piecewise constant, 30 pivot, 152 pivoting full, 152 partial, 152 Poincaré-Birkhoff-Witt Theorem, 36 polar decomposition, 382 polynomial, 38 characteristic, 239, 268 Chebyshev, 327 completely reducible, 43 cyclotomic, 42 in several indeterminates, 44 irreducible, 41 Jacobi, 327 Lagrange interpolation, 146 Legendre, 326 minimal, 248, 268 monic, 38 reducible, 41 zero, 38 polynomial function, 40 positive definite, 356 power exterior, 416 pre-Banach space, 309 pre-Hilbert space, 300 primitive root of unity, 136 process Arnoldi, 331 Gram-Schmidt, 328 product bra-ket, 121 cartesian, 2 cross, 36 direct, 19 dot, 300 dyadic, 130 exterior, 121 Hadamard, 157 inner, 299 interior, 121

433

Jordan, 37 ket-bra, 121 Kronecker, 413 Lie, 36 scalar triple, 306 Schur, 157 tensor, 411 vector triple, 306 projection, 104 onto an affine set, 342 orthogonal, 330 proper subspace, 22 pseudoinverse Moore-Penrose, 389 QR-decomposition, 335 quadratic form, 407 quadratic surface, 410 quasidefinite matrix, 366 quaternion algebra, 58 real, 58 range, 2 numerical, 409 rank, 89, 179, 403 Rational Decomposition Theorem, 274 rational number, 5 Rayleigh quotient function, 354 iteration scheme, 355 real euclidean, 299 real number, 5 real part, 7 real quaternion, 58 reduced row echelon form, 174 reducible, 41 relation equivalence, 106 partial order, 53 relaxation method, 188 restriction, 2 Riesz Representation Theorem, 338 right orthogonal complement, 403

434

Index

row echelon form, 173 row equivalent, 145 row space, 179 scalar, 18 scalar matrix, 132 scalar multiplication, 17 scalar triple product, 306 Schur product, 157 Schur’s Theorem, 371 selfadjoint, 349 semifield, 10 semisimple eigenvalue, 244 sequence, 2 Fibonacci, 269 linearly recurrent, 268 set difference, 2 generating, 25 partially-ordered, 53 spanning, 25 Sherman-Morrison-Woodbury Theorem, 138 signum, 203 similar matrices, 241 simple eigenvalue, 244 simple tensors, 410 singular matrix, 135 singular value, 383 Singular Value Decomposition Theorem, 382 skew symmetric matrix, 134 solution set, 171 solution space, 171 SOR, 188 space dual, 285 inner product, 300 normed, 309 pre-Banach, 309 pre-Hilbert, 300 solution, 171 spanning set, 25 sparse matrix, 187 special Lie algebra, 286

special orthogonal matrix, 375 spectral condition number, 383 Spectral Decomposition Theorem, 379 spectral norm, 311 spectral radius, 233 spectrum, 229 spline function, 48 Steinitz Replacement Property, 52 stochastic matrix, 135 Strassen-Winograd algorithm, 150 subalgebra, 35 unital, 35 subfield, 7 euclidean, 299 real euclidean, 299 subset affine, 86 bounded, 60 chain, 53 convex, 365 Hilbert, 332 orthonormal, 331 underlying, 2 subspace, 22 cyclc, 104 generated by, 25 improper, 22 invariant, 103 Krylov, 267 maximal, 292 nontrivial, 22 proper, 22 spanned by, 25 trivial, 22 subspaces disjoint, 23 independent, 67 pairwise disjoint, 24 successive overrelaxation method, 188 Sylvester’s Theorem, 89 symmetric bilinear transformation, 399 symmetric difference, 21

Index

symmetric matrix, 134 symmetric Toeplitz matrix, 183 system of linear equations, 169 homogeneous, 170 nonhomogeneous, 170 Taylor coefficient, 104 tensor algebra, 415 tensor product, 411 tensors entangled, 410 simple, 410 trace, 286 transcendental, 65 transform discrete cosine, 137 discrete Fourier, 136, 308 fast Fourier, 136 transformation affine, 86 bilinear, 399 linear, 79 opposite, 399 transpose, 85 conjugate, 301 Hermitian, 301 Triangle difference inequality, 307 Triangle inequality, 315 tridiagonal matrix, 133 trivial subspace, 22 underlying subset, 2 union, 2 unit, 34 unital algebra, 33 unital subalgebra, 35 unitarily similar matrices, 370 unitary automorphism, 369 unitary matrix, 370 upper Hessenberg matrix, 419 upper-triangular matrix, 133 Vandermonde matrix, 147 vector, 18 normal, 305

435

vector addition, 17 vector space, 18 finite dimensional, 63 finitely generated, 26 infinite dimensional, 63 vector triple product, 306 vectors orthogonal, 326 orthogonal with respect to a bilinear form, 403 wavelet Haar, 332 weak dual space, 290 weighted dot product, 301 Well Ordering Principle, 53 width of a band matrix, 133 word, 20 Wronskian, 207 Zlobec’s formula, 393 Zorn’s Lemma, 60

The linear algebra a beginning graduate student ought to know

The linear algebra a beginning graduate student ought to know

The Linear Algebra a Beginning Graduate Student Ought to Know